| Asymmetric particle emission in high energy cosmic ray interactions (p. 1) |
| by Wilczynski, H |
| OSSE observations spectra of X-rays pulsar (p. 1) |
| by Grove, J E |
| Measurement of electron and positron energy differential fluxes with MASS2 apparatus (p. 1) |
| by Basini, G |
| The plasma wake field exited by solar energetic flare electrons through the corona (p. 1) |
| by Huang, Y N |
| Study of intermittency in collisions of 4.5 A GeV/c Si with emulsion (p. 5) |
| by El-Naghy, A |
| Searching for the third Soft gamma repeater, SGR1900+14 (p. 5) |
| by Hurley, K |
| Flux of cosmic ray negatrons at 1.5 GeV (p. 5) |
| by Clem, J M |
| Relativistic electron spectrum and plasma wake field acceleration in large solar flares (p. 5) |
| by Huang Y N |
| Multiplicity characteristics of particles emitted in 4,5 A GeV/c Si - Emulsion collisions (p. 9) |
| by El-Naghy, A |
| Observations of cosmic ray positrons during the 1993 flight of the NMSU?Wizard - TS93 (p. 9) |
| by Aversa, F |
| Stochastic acceleration of electrons in localized wave fields (p. 9) |
| by Treumann, R A |
| A hard x-ray observation of Cyg X-1 in 1985 (p. 9) |
| by Ma, Y Q |
| Temporal variation of helium energy spectra and He He ratios for March and June 1991 SEP events (p. 12) |
| by Guzik, T G |
| Triggering of solar flares and particle acceleration (p. 13) |
| by Sakai, J |
| Multiplicities in nucleus-nucleus interactions at the highest accelerator energies (p. 13) |
| by Wolter, W |
| Soft X-ray excess in seyfert galaxies (p. 13) |
| by Piro, L |
| The cosmic positron fraction: implications of a new measurement (p. 13) |
| by Müller, D |
| Acceleration of solar particles by short wavelength (p. 14) |
| by Gallegos-Cruz, A |
| Study of some aspects of nucleus-nucleus interactions at (3-4.5) GeV/c (p. 17) |
| by El-Naghy, A |
| X-ray synchrotron emission from supernova-remnant shocks: constraints on shock-acceleration microphysics (p. 17) |
| by Reynolds, S P |
| A new measurement of the positron fraction at high energies (p. 17) |
| by Tarle, G |
| What can be learnt from H--, microwave and high energy emission of the march 26, 1991 solar flare? (p. 18) |
| by Kurt, V |
| Non-thermal emission from supernova remnants (p. 21) |
| by Mastichiadis, A |
| Energy-dependent propagation of high energy electrons (p. 21) |
| by Atoyan, AM |
| On multiparticle pseudorapidity correlations in central 4.5 A GeV/c C-Cu collisions (p. 21) |
| by Sarkisyan-Grinbaum, E |
| Ionization states of solar-flare particles (p. 22) |
| by Sakurai, K |
| Forward - backward correlations in nucleus-nucleus collisions at (4.1 - 4.5) A GeV/c (p. 25) |
| by El-Naghy, A |
| Is the galactic centre an obscured active galactic nucleus? (p. 25) |
| by Matt, G |
| The origin of cosmic ray positron (p. 25) |
| by Chi, X |
| Coulomb loss influence on the solar particle spectra at the stochastic acceleration (p. 26) |
| by Kartavykh, Yu |
| Investigation of high energy primary cosmic ray interaction with Pb and Fe Target nuclei in stratospheric emulsion chamber (p. 29) |
| by Apanasenko, A V |
| A model for X-ray and gamma-ray emissions from AGNs (p. 29) |
| by Wang, J M |
| Astrophysical significance of the confinement time of primary electrons in the galaxy (p. 29) |
| by Nishmura, J |
| Heavy ion acceleration with account of change transfer processes (p. 30) |
| by Kartavykh, Yu |
| The energy dependence of elasticity coefficient and cross-sections in hadron-lead interactions in the range 250 GeV-50 TeV (p. 33) |
| by Rakobolskaya, I V |
| Feedback mechanisms in AGN (p. 33) |
| by Mastichiadis, A |
| The thermal and non-thermal radio emission in the galactic disk and cosmic ray electron origin (p. 33) |
| by Osborne, J L |
| On the formation of relativistic particle beams in extended coronal structures: I. Evidences for two separate sources of solar cosmic rays (p. 34) |
| by Miroshnichenko, L I |
| Wavelet analysis of high multiplicity events (p. 37) |
| by Suzuki, N |
| The sax mission for wide band X-ray astronomy (p. 37) |
| by Piro, L |
| Demodulation of the interstellar positron/electron ratio in galactic cosmic rays (p. 37) |
| by Kneller, M |
| On formation of relativistic particle beams in extended magnetic structures: II. Two source model for solar cosmic rays (p. 38) |
| by Miroshnichenko, L I |
| Attenuation mean free path of high energy hadrons in lead (p. 41) |
| by Tamada, M |
| Performance of the SAX/PDS high energy X-ray telescope (p. 41) |
| by Frontera, F |
| A distributed acceleration model fitting simultaneously electrons and heavy ions (p. 41) |
| by Silberger, R |
| The origin in the corona of SEPs associated with CMEs (p. 42) |
| by Mendoza, B S |
| Cosmic ray electron spectra: prediction and data (p. 45) |
| by Wiebel-Sooth, B |
| Transverse momenta of helium fragments in gold fragmentation at 10.6 GeV/nucleon (p. 45) |
| by Wilczynska, B |
| A new balloon-borne detector for high angular resolution hard X-ray astronomy (p. 45) |
| by Cherry, M L |
| Distribution of SEP related flares in the solar disk (p. 46) |
| by Pérez-Enriquez, R |
| Propagation models for Cr nucleons and electrons and predictions of the galactic Gamma-ray spectrum (p. 48) |
| by Strong, A W |
| Interactions of 158 GeV/nucleon lead nuclei emulsion (p. 49) |
| by Deines-Jones, P |
| X-ray monitor for all sky (XMAS) mission (p. 49) |
| by Tümer, T O |
| Extremely high-energy solar protons by the data of Baksna underground scintillation telescope (p. 50) |
| by Karpov, S N |
| Low energy cosmic ray electrons: acceleration by weak shocks (p. 52) |
| by Skibo, J G |
| Nucleon-air nuclei interaction probability law and the inelastic cross-section (p. 53) |
| by Portella, H M |
| Morphological studies of short gamma ray bursts (p. 53) |
| by Bhat, P N |
| Absolute proton fluxes from the sun at rigidity above 1 GV by ground-based data (p. 54) |
| by Miroshnichenko, L I |
| Projectile fragmentation in Au+AI interactions at 0.930 GeV/n (p. 56) |
| by Bhattacharya, D P |
| Expected anisotropy of very high energy electrons (p. 56) |
| by Ptuskin, V S |
| A ROSAT look for the source of KeV emission following GRB780506 (p. 57) |
| by Connors, A |
| On the threshold effect of proton acceleration in solar flares (p. 58) |
| by Miroshnichenko, L I |
| Proton-proton total cross section derived from cosmic ray data (p. 60) |
| by Bellandi, J |
| Cosmic ray antiproton measurements in the 4-19 GeV energy range using the NMSU/Wizard-matter antimatter superconducting spectrometer 2 (MASS2) (p. 60) |
| by Hof, M |
| COMPTEL locations and spectra of ray bursts (p. 61) |
| by Kippen, R M |
| Upper intensity-energy limits and utmost spectrum for solar cosmic rays (p. 62) |
| by Miroshnichenko, L I |
| Production and detection of hyperfragments in high energy nucleus-nucleus collisions (p. 64) |
| by He, Y D |
| Cosmic ray antiproton observations from 0.2 to â 3.2 GeV (p. 64) |
| by Labrador, A W |
| The correlation between spatial distributions of GRBs and EAS super High energy (p. 65) |
| by Tkaczyk, W |
| Behavioural features of energy spectra of particle fluencies and peak fluxes in solar cosmic rays (p. 66) |
| by Nymmik, R A |
| Central high energy heavy nuclei collisions and ring-like effect (p. 68) |
| by Chernavskaj, O D |
| Interpretation of the low-energy cosmic ray antiproton/proton ratio (p. 68) |
| by Labrador, A W |
| LogN-LogP and space distribution of GRBs (p. 69) |
| by Belli, B M |
| Sectorial distribution of LDE-type flares (p. 70) |
| by Antalova, A |
| Cosmic ray antiproton observations by the isotope matter-antimatter experiment : 0.2 to 3.2 GeV(p. 72) |
| by Mitchell, J W |
| Search for low energy and in coincidence with BATSE gamma ray bursts (p. 73) |
| by Aglietta, M |
| The particles source temperatures in the Fe-rich and Fe-poor events (p. 74) |
| by Wang, X Y |
| The model of the interaction of leptons with the nuclei in the presence of the superhigh energies (p. 76) |
| by Khazaradze, N G |
| Observation of antiprotons at low energies by BESS detector (p. 76) |
| by Orito, S |
| VHE gamma ray astronomy and gamma ray bursts (p. 77) |
| by Hurley, K |
| Post-eruption particle acceleration in the corona: a possible contribution to solar cosmic rays (p. 78) |
| by Chertok, I M |
| Energy dependence of particle multiplicities from p-p collisions (p. 80) |
| by Liland, A |
| p(-) and e+ identification capabilities of CAPRICE (p. 80) |
| by Barbiellini, G |
| Scaling laws for generation of high-energy secondary emission in magnetic loops (p. 82) |
| by Kocharov, L G |
| A double-core event detected at Chacaltaya (p. 84) |
| by Amato, N M |
| Likelihood methods and classical burster repetition (p. 84) |
| by Graziany, C |
| Antiproton proton ratio at 10 eV inferred from the superposition of sun shadows using the Tibet air shower (p. 84) |
| by Amenomori, M |
| Solar cosmic ray events: statistical characteristics for the diagnostic of acceleration, escaping and propagation processes (p. 86) |
| by Dorman, L I |
| Multi-particle correlations in S+Pb and Pb+Pb interactions at CERN SPS energies (p. 87) |
| by Takahashi, Y |
| A burst of pulsed VHE rays from AE aquarii (p. 88) |
| by Chadwick, P M |
| Calculation of the charged pion albedo from the moon regolith induced by cosmic antiprotons (p. 88) |
| by Brunetti, M T |
| Small-Scale acceleration processes in solar flares during primary energy release phase (p. 90) |
| by Pissarenko, N F |
| A search for cosmic ray antihelium with BESS (p. 92) |
| by Ormes, J F |
| Search for 10TeV ray bursts with the Tibet air shower array (p. 92) |
| by Amenomori, M |
| The temporal and spectral characteristics of solar gamma-flares on the data of gamma-1 (p. 94) |
| by Djantemirov, H M |
| Searches for TeV rays in classical gamma-ray bursts (p. 96) |
| by Connaughton, V |
| Partial lifetimes of antiprotons from diffuse radiation (p. 96) |
| by Stephens, S A |
| Downward beaming of ions and electrons in the 1991 November 15 flare (p. 98) |
| by Yoshimori, M |
| The highest energy cosmic rays and the fluctuations in the cosmic microwave background (p. 99) |
| by Roy, S |
| Search for short time emission in the UHE range above 20 Tev with the HEGRA detector (p. 100) |
| by Padilla, L |
| Simulation code for the propagation of cosmic rays in the Milky Way (p. 100) |
| by Codino, A |
| Spectral characteristics of solar gamma-ray flares (p. 102) |
| by Yoshimori, M |
| Production of heavier particles than pions in fire-balls (p. 103) |
| by Augusto, C R A |
| Search for TeV-gamma rays from evaporating primordial black holes (p. 104) |
| by Funk, B |
| Propagations of cosmic rays in the galaxy (p. 104) |
| by Doi, T |
| Temporal evolution of X-and rays during a flare on 27 October 1991 (p. 106) |
| by Kotov, Yu D |
| Abrasion-evaporation model and cosmic ray nuclei interactions (p. 107) |
| by Capdevielle, N |
| Search for TeV counterparts of 1994 and 1995 BATSE rays bursts (p. 108) |
| by Krawczynski, H |
| On using the weighted slab approximation in studying cosmic-ray transport (p. 108) |
| by Ptuskin, V S |
| On the beaming of solar flare energetic photons (p. 110) |
| by Li, P |
| Comparison of some methods of calculating differential cross sections for the production of in PP-interactions at (4.5-1800)GeV (p. 111) |
| by Uryson, A V |
| Search for 10 TeV gamma bursts from evaporating primordial black holes with the Tibet air shower array (p. 112) |
| by Amenomori, M |
| Cosmic ray perpendicular diffusion: approach based on the Ito equation (p. 112) |
| by Klepach, E G |
| Measurements of the duration of particle emission from solar flares (p. 114) |
| by Ruffolo, D |
| Kilometric radiation connected with trap-loop structure of the interplanetary magnetic field (p. 115) |
| by Grigorieva, V P |
| Study of the high energy cosmic ray cascades using the dual parton model (p. 115) |
| by Battistoni, G |
| Search for an ultra high energy component of gamma-ray bursts (p. 116) |
| by Borlone, A |
| Hydrodynamic approach to cosmic ray propagation (p. 116) |
| by Ko, C M |
| He and heavy ion enhancements in impulsive solar flares due to EMIC wave (p. 118) |
| by Roth, I |
| Fragmentation of 160 A GeV Pb in various targets (p. 119) |
| by He, Y D |
| A search for TeV and PeV gamma Ray bursts (p. 120) |
| by Edwards, P G |
| A 3D-model for the propagation of cosmic rays (p. 120) |
| by Pohl, M |
| Heavy-ion acceleration beyond 10 MeV/nucleon in impulsive solar flares: SAMPEX observations (p. 122) |
| by Mazur, J E |
| The predictions of quark-gluon string model and the data of air showers at ultra high energies (p. 123) |
| by Kalmykov, N N |
| Galactic cosmic ray propagation at low energies: the interstellar medium and partial cross sections (p. 124) |
| by Thayer, M R |
| Time evolution of solar proton energy spectra at the earth orbit and possibility of multi-step particle acceleration (p. 127) |
| by Belov, A |
| Search for UHE gamma ray counter-parts of GRB's (p. 128) |
| by Bhat, P N |
| Diffusion of cosmic rays in strongly inhomogeneous magnetic field (p. 128) |
| by Ptuskin, V S |
| Effect of deformed target nucleus on abration and absorption cross sections (p. 131) |
| by Ramadan, S |
| GOES response to energetic protons of different origin (p. 131) |
| by Vainio, R |
| Search for gamma rays bursts of energy E 10 GeV and E 100TeV (p. 132) |
| by Vernetto, S |
| Decaying cosmic ray nuclei as a probe of the of the local interstellar medium (p. 132) |
| by Ptuskin, V S |
| A microscopic eikonal-type model for electron-proton scattering (p. 135) |
| by Hussein, M T |
| Energetic protons from the 1990 May 24 solar flares as detected by GOES satellites (p. 135) |
| by Torsti, J |
| Transport of ultra-high energy cosmic rays in galactic magnetic fields (p. 136) |
| by Pochepkin, D N |
| A multi-cluster model in hadron nucleus interactions at high energies (p. 139) |
| by Hussein, M T |
| Successive solar energetic particle events in the October 1989 (p. 139) |
| by Torsti, J |
| Searching for gamma-ray bursts with water-Cherenkov-detector (p. 140) |
| by Allen, G E |
| The interpretation of ultra heavy cosmic ray data by the halo diffusion model (p. 140) |
| by Jansen, F |
| A Monte-Carlo generator of mini-jet model for the simulation of hadron multiproduction (p. 143) |
| by Cheung, T |
| Solar neutron decay proton (p. 143) |
| by Sakai, T |
| Setting Up a calculation method based on the leaky box model for ultra heavy cosmic ray propagation (p. 144) |
| by Font, J |
| Consequences of disoriented Chiral condensates in EAS properties (p. 147) |
| by Capdevielle, J N |
| The June 3, 1982 solar flares as a test for neutron monitor sensitivity for solar neutrons (p. 147) |
| by Kananen, H |
| Origin of the structure in gamma ray bursts (p. 148) |
| by Chan, H Y |
| Isotopes decaying by K-capture as a probe of reacceleration-deceleration of low energy cosmic rays (p. 148) |
| by Soutoul, A |
| Fluctuations and correlations beyond midrapidity (p. 151) |
| by Wilk, G |
| High energy neutrons from the June 15, 1991 solar flare as detected by the neutron monitor (p. 151) |
| by Usoskin, I G |
| Ray bursts from planetoid accretion onto fast galactic neutron stars (p. 152) |
| by Colgate, S A |
| The anisotropy of low energy cosmic rays and properties of the local interstellar medium (p. 152) |
| by Fatemi, J |
| Cosmic-ray rapidity density distribution and super-families (p. 155) |
| by Costa, C G |
| Two injections of high energy neutrons during the May 24, 1990 solar flare (p. 155) |
| by Kovaltsov, G A |
| Gamma jets by processing neutron star jets in galactic binary systems, GRBs (p. 156) |
| by Fargion, D |
| On the anisotropy of the higest energy cosmic rays from the galactic centre (p. 156) |
| by Zielinska, M |
| Lateral spread of hadronsin high-energy super-families and centauro events (p. 159) |
| by Costa, C G |
| Correlative investigations of the 1990 May 24 solar flare (p. 159) |
| by Kocharov, L G |
| Cosmic-ray-modified shocks with injection (p. 160) |
| by Chan, K W |
| Fire-balls masses seen in C-jets (p. 163) |
| by Augusto, C R A |
| Search for neutron decay protons from the 1990 May 24 solar flare (p. 163) |
| by Kocharov, L G |
| Merger models of gamma-ray bursts: a comparison (p. 164) |
| by Sivaram, C |
| Production of galactic antiprotons under diffuse reacceleration (p. 164) |
| by Simon, M |
| Gamma-ray burst and the leftovers of star bursts in active galactic nuclei (p. 166) |
| by Steiner, J E |
| Comments to short mean free path particles observed by Pamir thick lead chambers (p. 166) |
| by Ohsawa, A |
| The relationship between the timing of solar flare ray emission and high-energy neutron production (p. 167) |
| by Debrunner, H |
| Oxygen fragmentation cross sections (p. 168) |
| by Isbert, J |
| Alignment of energy distinguished cores in families and hadron aspects of the phenomenon (p. 170) |
| by Kopenkin, V V |
| Search for MeV emission from The X-ray binary Cyg X-3 (p. 170) |
| by Collmar, W |
| Comment on the minimum mass path of a uni-directional solar neutron particle beam through the earth atmosphere (p. 171) |
| by Smart D F |
| Fragmentation of 10.6 GeV/nucleon gold nuclei on a hydrogen target (p. 172) |
| by Holynski, R |
| Explanation of the appearance as if exotic phenomena on hadron attenuation in deep lead chambers in the frame of two-component model of high energy hadrons interaction (p. 174) |
| by Smirnova, M D |
| OSSE and EGRET observations of the crabe and vela supernova remnants (p. 174) |
| by De Jagger, O C |
| Simultaneous observations of solar neutrons of June 6, 1991 at Mt. Haleakala and Mt. Norikura (p. 175) |
| by Muraki, Y |
| Measurements of fragmentation cross sections with heavy ion beams below 1 GeV/nucleon (p. 176) |
| by Cassagnou, Y |
| The FWHM of the transition curves of showers and the identification of hadrons and gamma-rays in Fe-emulsion chambers (p. 178) |
| by Fu, Y |
| Diffuse ray emission in the outer galaxy from the cepheus flare and the perseus arm (p. 178) |
| by Grenier, L A |
| Comments on second and third enhancements of solar particles on June 4, 1991 flare (p. 179) |
| by Muraki, Y |
| Experimental and simulated characteristics of âﾜhaloâ in superfamilies with primary energy higher than 10 PeV (p. 182) |
| by Borisov, A S |
| EGRET observations of the galactic plane diffuse radiation and implications for the cosmic ray electron to proton ratio (p. 182) |
| by Hunter, S D |
| Probable detection of electrons from the decay of solar flare neutrons (p. 183) |
| by Dröge, W |
| Systematics of new isotopic production cross sections from neon projectiles (p. 184) |
| by Chen, C X |
| The attenuation of high energy hadrons in iron (p. 186) |
| by Ren, J R |
| Solar energetic electrons: I. Multiple spacecraft observations (p. 187) |
| by Dröge, W |
| Charge changing cross sections near the - isobar resonance (p. 188) |
| by Doll, P |
| The intensity of super high energy gamma-rays at the altitude of Yangbajing (p. 190) |
| by Ren, J R |
| Search in the EGRET 50Mev-30 GeV data for emission from previously claimed VHE sources (p. 190) |
| by Merck, M |
| Solar energetic electrons: II. Comparison with ray emission (p. 191) |
| by Dröge, W |
| Nuclear interaction cross sections for ultra-heavy nuclei (p. 192) |
| by Garrard, T L |
| The effect of Narrow gamma families from the data of experiment PAMIR (p. 193) |
| by Zhdanov, G B |
| Emission of high energy gamma rays from six pulsars (p. 195) |
| by Metrck, M |
| The observation of solar flare protons with energy more than 30 MeV in vicinity of the earth on board station âﾜMIRâ on 30 October 1991 (p. 195) |
| by Galper, A M |
| The study of galactic cosmic ray CNO source abundances using new isotope cross sections (p. 196) |
| by Guzik, T G |
| Single Pion momentum spectrum up to 2 TeV (p. 197) |
| by Mielke H H |
| Structure and variability of the crab Pulsar Light curve in the X and ray bands (p. 199) |
| by Massaro, E |
| Solar cosmic rays and solar activity cycles (p. 199) |
| by Nazarova, M N |
| Abundance of the low energy isotopes of carbon nitrogen and oxygen at the cosmic ray (p. 200) |
| by Soutoul, A |
| Nuclear interaction families associated to EAS at Mt. Chacaltaya (p. 201) |
| by Kawasumi, N |
| High energy neutrons and rays from the solar flare of 1991 June 11 (p. 203) |
| by Dunphy, P P |
| COMPTEL observations of millisecond pulsar (p. 203) |
| by O'Flaherty, K S |
| Accelerated particle Spectrum during the solar system formation (p. 204) |
| by Ustinova, G K |
| The 2.223 Mev gamma line time dependence as a probe of density inhomogeneity of solar atmospheric and subphotospheric layers (p. 204) |
| by Kuzhevskj, B |
| On lateral distribution of oblique electromagnetic cascade (p. 205) |
| by Kolchushkin, A M |
| COMPTEL limits on 1,8 MeV gamma-ray line emission from the Orion region (p. 207) |
| by Oberlack, U |
| Pecullarities of characteristics of interaction of relativistic nuclei with nuclei Ag. Br. (p. 208) |
| by Adamovich, M I |
| Comparison of ground-Level enhancements of 15 November 1960 and 22 october 1989 (p. 208) |
| by Shea, MA |
| On fluctuations of electromagnetic shower axix (p. 209) |
| by Chernov, D E |
| Early results from the investigation of nuclear fragmentation of relativistic ultra Heavy (p. 211) |
| by Thompson, A |
| Diffuse galactic gamma-ray emission (p. 211) |
| by Purcell, W R |
| The lateral electron distribution in electromagnetic showers in atmosphere (p. 212) |
| by Goncharov, A I |
| The GLE of September 29, 1989: analysis of the pitch angle distribution I (p. 212) |
| by de Koning, C A |
| Time Dependent shock acceleration (p. 212) |
| by Axford, W I |
| Identification of the CGRO source j2021+37 with the open cluster Berkeley 87 (p. 215) |
| by Polcaro, V F |
| Cerenkov radiation from EAS: influence of absorption in ozone on the observations in UV range (p. 216) |
| by Attallah, R |
| The GLE of September 29, 1989: analysis of the pitch angle distribution II (p. 216) |
| by de Koning, C A |
| Diffusive shock acceleration in dense and incompletely ionized media (p. 217) |
| by O'Connor-Drury, L |
| Implications of the OSSE and COMPTEL observations of the diffuse galactic gamma rayu continuum (p. 219) |
| by Skibo, J G |
| Anisotropic space distribution of solar particles of the GLE observed on 24 May 1990 (p. 220) |
| by Morishita, L |
| Compound diffusion and particle acceleration at shocks (p. 221) |
| by Dendy, R O |
| Application of a Bayesian method to COMPTEL pulsar data (p. 223) |
| by Connors, A |
| The correlation analysis of gamma-families originated in pA and AA interactions at the superhigh energies E 10 eV (p. 224) |
| by Yuldashbaev, T S |
| The phenomenology of the precursor increase on the 19 October 1989 ground level event (p. 224) |
| by Stoker, P H |
| The influence of particle scattering on acceleration rates and injection efficiencies in oblique shocks (p. 225) |
| by Ellison, D C |
| A search for radio-Quiet gamma-ray pulsars in the EGRET archive (p. 227) |
| by Koh, T |
| Halo events in super high energy nuclear interactions (p. 228) |
| by Ren, J R |
| The solar cosmic ray event of June 4-19, 1991 according to the granat spacecraft data (p. 228) |
| by Chuchkov, E A |
| Spectral comparison of Monte Carlo Simulations of particle acceleration with Ulysses observations of nearby interplanetary shocks (p. 229) |
| by Baring, M G |
| The preliminary cosmic diffuse ray spectrum from 800 keV to 30 MeV measured with COMPTEL (p. 230) |
| by Kappadath, S C |
| Simulation studies related to TACTIC and MYSTIQUE ray telescopes (p. 232) |
| by Gandhi, V N |
| The GLE of 29 September 1989. Time variations of the cosmic-ray rigidity spectrum (p. 232) |
| by Dvornikov, V M |
| Nonlinear plasma effects in cosmic ray shock precursors (p. 233) |
| by Dendy, R O |
| The spectrum of diffuse galactic continuum gamma rays measured by COMPTEL (p. 234) |
| by Strong, A W |
| A study of shower transition behaviours initiated by hadron-pb interaction (p. 236) |
| by Tamada, M |
| The GLE of 29 September 1989. Time variations in angular distribution of different-energy particles (p. 236) |
| by Dvornikov, V M |
| Limits on the time variability of ion injection in quasi-parallel shocks (p. 237) |
| by Bennett, L |
| Possible break in the spectrum of the diffuse gamma ray emission at the energy E 100 GeV (p. 238) |
| by Uryson, A V |
| Simulation of hadronic cascades including vacuum excitation and higgs production (p. 240) |
| by Boruah, K |
| High energy particle generation during the solar flares (p. 240) |
| by Kolomeets, E |
| Non thermal electron injection by collisionless shock waves (p. 241) |
| by Bykov, A M |
| Multiwavelengh observations of the blazer PKSO521-365 (p. 242) |
| by Smith, N |
| A study of LPM suppression of bremsstrahlung at 25 GeV (p. 243) |
| by Kelley, L |
| Review of ground-level solar cosmic ray enhancements during the 22nd solar cycle (p. 244) |
| by Shea, M A |
| Diffusive particle acceleration in oblique shocks : comparison of numerical results with observations(p. 245) |
| by Jones, T W |
| Azimuthal peculiarities of gamma-ray-hadron families and new physics at 4 TeV (p. 247) |
| by Mukhamedshin, R A |
| Neutron monitor responses during highly anisotropic ground level enhancements (p. 248) |
| by Cramp, J L |
| Cosmic ray acceleration by pulsar wind (p. 249) |
| by Giller, M |
| An attempt to detect a ray halo around the Virgo cluster (p. 250) |
| by Fatemi, J |
| Confinment violation at 3.10 cm and nucleon interactions in energy interval of 10 - 10 eV (p. 251) |
| by Nikolsky S I |
| Complex features of the GLE of 29 september 1989 (p. 252) |
| by Xue, S S |
| Implications of ray lines observed from the Orion complex. II (p. 253) |
| by Cowsik, R |
| Particle acceleration of relativistic shock waves in electron-ion plasmas (p. 253) |
| by Hoshino, M |
| Interplanetary transport coefficient in an extended quasi-linear theory (p. 253) |
| by Ng, C K |
| Do emulsion chamber double-core events manifest quark composition (p. 255) |
| by Popova, L |
| Gam,ma-rays from the Orion star-forming complex (p. 256) |
| by Erlykin, A D |
| Extreme âﾜpropagationâ of solar energetic particles (p. 257) |
| by Cliver, E W |
| Cosmic ray acceleration time scale at relativistic shock waves (p. 257) |
| by Ostrowski, M |
| The influence of charm production on cascades induced by cosmic ray hadrons in lead at energy 20-200 TeV and in atmosphere at energy 500 TeV-500 PeV (p. 258) |
| by Dunaevsky, A M |
| Simulation of the annihilation spectrum of a massive black hole in the galactic center (p. 260) |
| by Fenyves, E J |
| Relativistic shock acceleration speed-up: allowance for non-linear effects (p. 261) |
| by Quenby, J J |
| Pitch angle distribution of solar energetic particles (SEPs) and the transport parameters in interplanetary space, I: properties of steady-state distributions (p. 261) |
| by Hatzky, R |
| Study of fragmentation process of Si nuclei in emulsion at 4,5 A GeV/c (p. 262) |
| by El-Naghy, A |
| Probable gamma-ray line spectrum from an accreting neutron star (p. 263) |
| by Bardoloi, I |
| Monte Carlo simulation of diffusive particle acceleration in oblique shock waves (p. 265) |
| by Naito, T |
| Pitch angle distribution of solar energetic particles (and the transport parameters in interplanetary space, II: local scattering properties (p. 265) |
| by Hatzky, R |
| Can photons with energies 10 eV pass the earth's magnetosphere ? Analysis of the observed highest energy cosmic rays (p. 266) |
| by Karakula, S |
| Annihilation lines from galactic BH candidates (p. 267) |
| by Pohl, M |
| Renormalized twoo-fluid hydrodynamics of cosmic ray modified shocks (p. 268) |
| by Malkov, M A |
| Turbulence and the quasilinear theory âﾜ Discrepancy âﾜ (p. 269) |
| by Bieber, J W |
| The MOCCA program: Monte-Carlo cascades (p. 270) |
| by Hillias, A M |
| Photon splitting in neutron star magnetospheres (p. 271) |
| by Baring, M W |
| Hadronic component in maximum air shower development observed at Mt. Chacaltaya (p. 273) |
| by Inoue, N |
| Electrostatic shocks driven by accelerated electrons (p. 273) |
| by Malkov, M A |
| Solar energetic protons self generated waves in the interplanetary magnetic field ( A search for evidences ) (p. 273) |
| by Valdés-Galicia, J F |
| Soft diffuse galactic ray continuum generated by CR Electrons (p. 275) |
| by Dogiel, V A |
| EASs showing chaotic feature over very long distance (p. 277) |
| by Chikawa, M |
| Injection of thermal particles at parallel shocks (p. 277) |
| by Malkov, M A |
| Propagation of coherent pulses of solar cosmic rays (p. 277) |
| by Ruffolo, D |
| The injection rate of e Pairs by relativistic nuclei in magnetospheres of young pulsars (p. 279) |
| by Bednarek, W |
| Zenith angle dependence on depth of shower maxima (p. 281) |
| by Nath, D |
| The excitation of ion cyclotron harmonic waves in cosmic ray shock precursors (p. 281) |
| by McClements, K G |
| Ulysses, Voyager 1 and IMP-8 low energy proton fluxes: Interplanetary particle transport (p. 281) |
| by Anglin, J D |
| Multiwavelength spectral modeling of blazars (p. 283) |
| by Dermer, C D |
| The knee of the size spectrum of EAS at different depths in the atmosphere (p. 285) |
| by Danilova, E V |
| The spectral index of accelerated particles in oblique shock waves (p. 285) |
| by Naito, T |
| Rigidity dependent pitch angle distribution in modeling ground level enhancements (p. 285) |
| by Cramp, J L |
| Chaotic feature of extensive cosmic ray air showers (p. 289) |
| by Ohara, S |
| Test particle energy gains at oblique shocks using the adiabatic approximation (p. 289) |
| by Baring, M G |
| The effect of near-earth IMF structure on the modeling of ground level enhancements (p. 289) |
| by Cramp, J L |
| The superluminal factor of gamma ray blazars (p. 291) |
| by Chi, X |
| Study of the EAS cores from the EAS-TOP calorimeter and observation of multi-core events (p. 293) |
| by Antonioli, P |
| The cosmic ray spectrum and irregularities of galactic magnetic field (p. 293) |
| by Tkaczyk, W |
| Propagation of charged particle pulses immediately after injection (p. 293) |
| by Earl, J A |
| Production of gamma-rays in blazers by electrons accelerated in the jet (p. 295) |
| by Bednarek, W |
| First experimental results from the array of cascade (p. 297) |
| by Schieler, H |
| Solar cosmic ray transport under anisotropic injection (p. 297) |
| by Fedorov, Yu I |
| The extragalactic diffuse ray emission and radiative neutrino decay (p. 299) |
| by Miller, R S |
| Fractal study of extensive air shower time series (p. 301) |
| by Katayose, Y |
| Origin of the high energy extragalactic ray background (p. 303) |
| by Wolfendale, Arnold Whittaker |
| Simulations of cosmic ray cross field diffusion (p. 305) |
| by Ostrowski, M |
| Search for bursts of extensive air shower (p. 305) |
| by Katayose, Y |
| Spectral dependence on solar corona propagation of relativistic solar flare protons (p. 305) |
| by Stoker, P H |
| Signature of baryon symmetric universe and lifetime of antiprotons (p. 307) |
| by Stephens, S A |
| Charged particles separation in EASY by the geomagnetic field (p. 309) |
| by Dedenko, L G |
| a comment on the detection of solar proton events at the earth with respect tot the helliopheric current sheet (p. 309) |
| by Shea, A |
| High energy gamma rays from SN 1006 AD (p. 311) |
| by Damon, P E |
| Spectra of gamma-hadron families combined with EAS (experiment âﾜ hadron âﾜ) (p. 313) |
| by Cherdyntseva, K V |
| Wave-wave interactions in two fluid cosmic ray hydrodynamics (p. 313) |
| by Webb, G M |
| The heliolongitudinal distribution of solar flares associated with solar proton events (p. 313) |
| by Smart, D F |
| The crab gamma ray spectrum over 2 TeV (p. 315) |
| by Djannati-Atai, A |
| Fractal analysis of particle density distribution in extensive Air showers (p. 317) |
| by Kempa, J |
| The turbulence environment of stellar superbubbles and the implications for Fermi acceleration (p. 317) |
| by Spangler S R |
| Peculiarities of Anisotropy during ground level events of 22 cycle of solar activity (p. 317) |
| by Vashenyuk, E V |
| Observations of the crab Nebula with the second HEGRA Cherenkov telescope (p. 319) |
| by Deckers, T |
| A study of large-zenith-angle air showers with the CYGNUS experiment (p. 321) |
| by Allen, G E |
| Conservation laws and similary solutions in two fluid cosmic ray hydrodynamics (p. 321) |
| by Webb, G M |
| Injection and transport of accelerated particles as deduced from GOES and neutron monitor data (p. 321) |
| by Vainio, R |
| Search for emission of periodic TeV gamma rays from the crab Nebula and Geminga (p. 323) |
| by Gillanders, G B |
| Core structure of EAS above 10eV at Akeno (p. 325) |
| by Sakuyama, H |
| Short wavelength vorticity and contact modes in two fluid cosmic ray hydrodynamics (p. 325) |
| by Webb, G M |
| Coronal and interplanetary magnetic sector structure and the modulation of solar energetic particle events (p. 325) |
| by Kahler, S W |
| Observations of crab at low elevation using the pulse shape technique (p. 327) |
| by Patterson, J R |
| Azimuthal angular distribution for EAS between 1-10 TeV energies (p. 328) |
| by Aliaga, Z |
| Anisotropy of the cosmic rays in model with randomly distributed discrete galactic (p. 329) |
| by Lagutin, A |
| Numerical simulations and analytic theory of cross-field transport (p. 329) |
| by Jokipii, J R |
| The search for gamma cosmic rays from crab direction for the TeV energies (p. 330) |
| by Aliaga, Z |
| The transverse momentum of hadrons in extensive air showers (p. 332) |
| by Arvela, H |
| Transport coefficients in stochastic magnetic fields (p. 333) |
| by Kota, J |
| High energy gamma-ray from crab Nebula and Markarian 421 from the wide angle mirror Cerenkov telescope SHALON at the Mountain altitudes experiment SHALON-ALATOO (p. 334) |
| by Sinitsyna, N N |
| The hadron component in extensive air showers (p. 336) |
| by Arvela, H |
| Spectrum of ultra-high energy cosmic rays acceleration in superbubbles (p. 337) |
| by Bykov, A M |
| Some properties of fully three-dimensional drift model for the modula (p. 337) |
| by Hattingh, M |
| The location of the VHE Gamma-ray radiation regions in the crab Nebula (p. 338) |
| by Chalenko, N N |
| Delayed pulses observed in extensive air showers (p. 340) |
| by Arvela, H |
| The coherent acceleration of ultra high energy cosmic rays and the galactic dynamo (p. 341) |
| by Colgate, S A |
| Comparisson of three numerical treatments of charged particle transport (p. 341) |
| by Earl, J A |
| VHE Observations of the Crab Nebula from the Cherenkov array of EAS-TOP (p. 342) |
| by Aglietta, M |
| The experimental set-up and air shower measurements performed with the Turku air shower array (p. 344) |
| by Elo, A M |
| On galactic and metagalactic cosmic rays (p. 345) |
| by Ginzburg, V L |
| Revised Landau damping rates of ion-cyclotron waves and electron-cyclotron waves in hot equilibrium plasmas (p. 345) |
| by Schlickeiser, R |
| Search for steady Emission of 10 TeV gamma rays from the crab Nebula and Markarian 421 using the Tibet air shower array (p. 346) |
| by Amenomori, M |
| Statuts report on âﾜ Maket-Aniâ experiment (p. 348) |
| by Avakian, V V |
| Origin of cosmic rays at energies above 100 Tev (p. 349) |
| by Shoji Dake |
| Shock drift acceleration of electrons (p. 349) |
| by Vandas, M |
| A search for ultrahigh energy gamma-ray emission from the crab Nebula (p. 350) |
| by Borione, A |
| Single-particle arrival-time Pdf and related functions describing EAS fronts (p. 352) |
| by Linsley, J |
| Acceleration of highest energy (>10 20 eV) cosmic rays by superconducting cosmic strings (p. 352) |
| by Sivaram, C |
| Can diffusive shock acceleration work fast enough in interplanetary shocks? Evidence from the November 1992 event (p. 353) |
| by Lim, T L |
| Search for the crab Nebula and Mrk 421 with an improvided sensitivity and a lower energy threshold of the HEGRA arrays (p. 354) |
| by Prahl, J |
| Time-track complementary revisited (p. 356) |
| by Linsley, J |
| Possible astrophysical sources for the highest energy cosmic rays (p. 356) |
| by Sigl, G |
| The self-consistent model for acceleration of solar wind protons by the interplanetary shock waves and coupled alfven wave generation (p. 357) |
| by Berezhko, E G |
| On the GAMMa-ray emission mechanisms in the crab Nebula (p. 358) |
| by Aharonian, F A |
| Production height distribution of Eas muons given by the Palermo-Leeds-Napoli track time experiment (p. 360) |
| by Catalano, O |
| Can the highest energy cosmic rays also be of galactic origin? (p. 360) |
| by Wdowczyk, J |
| The Palermo-Leeds-Napoli Track time experiment (p. 361) |
| by Agnetta, G |
| Injection rate of shock- accelerated particles at the cobpoint: Dependence on thee heliolongitude (p. 361) |
| by Sanahuja, B |
| Lateral distribution of Eas particles given by Rpc detectors in the Palermo-Leeds-Napoli track time experiment (p. 362) |
| by Agnetta, G |
| to cosmic rays flux ratio from crab Nebula in the energy range 1 - 10 TeV (p. 362) |
| by Badran, H M |
| Estimating the significance of EAS double fronts (p. 363) |
| by Catalano, O |
| Arrival time distribution of EAS particles given by the Palermo-Leeds-Napoli track time experiment (p. 364) |
| by Agnetta, G |
| Integral EAS spectrum at mountain altitude in the âﾜKneeâ region (p. 365) |
| by Ter-Antonian, S V |
| Multispacecraft studies of coronal Mass ejection associated energetic particle events (p. 365) |
| by Barbier, L M |
| Upper limits on TeV gamma-ray emission from EGRET-detected GeV gamma-ray sources (p. 366) |
| by Quinn, J |
| High energies particles from the surface of a rotating cosmic magnet (p. 368) |
| by Thielheim K O |
| Energy spectrum and hadron lateral distribution in EAS at mountain altitude, Maket-Ani experiment (p. 369) |
| by Ter-Antonian, S V |
| Magnetic traps in the interplanetary medium connected with magnetic clouds (p. 369) |
| by Vandas, M |
| On the flaring activity of AE aquari in the radio, optical and VHE Gamma-rays (p. 370) |
| by Atoyan, A M |
| Maximum energy of CR accelerated by supernova shocks (p. 372) |
| by Berezhko, E G |
| Separation of gamma and proton showers (1-10 TeV) using the lateral distribution of Cerenkov light at several observatory Depths (p. 373) |
| by Pontocarrero, C |
| Anisotropies of solar particle onset observed within ejecta (p. 373) |
| by Richardson, I G |
| Recent observations of vela X 1 made with the university of Durham Mark 3A VHE ray (p. 374) |
| by Chadwick, P M |
| On the cosmic-ray flux inside the geminga supernova remnant (p. 376) |
| by Johnson, P A |
| Horizontal air showers: The role of fluctuations (p. 377) |
| by Parente, G |
| The response of energetic particles to the presence of ejecta material (p. 377) |
| by Cane, H V |
| A search for TeV emission from AE aquari (p. 378) |
| by Lang, M J |
| Cosmic rays and gamma rays in supernova remnants (p. 380) |
| by Berezhko, E G |
| A search for VHE emission from AE Aquari (p. 381) |
| by Bradbury, S M |
| The observation of low energy ions accelerated by an interplanetary shock on February 21st 1994 with the geotail HEP experiment (p. 381) |
| by Koi, T |
| Development of nucleus-air-nucleus interactions model to study the structure of EAS front (p. 381) |
| by Popova, L |
| Preferential acceleration and the origin of R-process nuclei (p. 384) |
| by Binns, W R |
| A new Vhe gamma-ray source in the Cygnus constellation (p. 385) |
| by Neshpor, Yu, I |
| Do âﾜTypicalâ low-energy ESP events exist? (p. 385) |
| by Lario, D |
| Calculation of air shower profiles using a bootstrap el;ectromagnetic bootstrap program (p. 386) |
| by Stanev, T |
| Study of electrons simultaneously with muons in extensive air showers (EAS) initiated by primary cosmic rays of energy 10 -10 eV (p. 387) |
| by Chakrabarti, C |
| Unpulsed high energy gamma-rays from a Plieronic Nebula (p. 387) |
| by Yoshida, T |
| CNOF isotopic abundances during thermonuclear gamma-ray bursts: A probable source of cosmic radiation (p. 388) |
| by Bardoloi, I |
| The detection of the VHE gamma-ray burst in the Vicinity of the red dwarf star EV lac (p. 389) |
| by Alekseev, I Yu |
| An electron Fermi acceleration event at an interplanetary shock wave on Feb. 21, 1994 GEOTAIL observation (p. 389) |
| by Terasawa, T |
| A comparative study of EAS energy estimation methods (p. 391) |
| by Chilingarian, A A |
| Chemical composition of cosmic rays accelerated in supernova remnants (p. 392) |
| by Berezhko, E G |
| Observations of pulsars near 1 Tev by the Cangaroo Project (p. 393) |
| by Kifune, T |
| The 11980 interplanetary particles anomalous perios and the solar magnetic activity (p. 393) |
| by Rodriguez-Pacheco, J |
| The energy estimates of EAS and the composition and energy spectrum of the primary particles at energies of 10 -10 eV (p. 395) |
| by Anokhina, A M |
| Ultra heavy nuclei in the source composition of cosmic rays (p. 396) |
| by Sakurai, K |
| Temporal behavior of different energy (<60 Kev, > 1 Mev) particle fluxes during cycle 21 maximum (p. 397) |
| by Rodriguez-Pacheco, J |
| Introduction to cosmos and some relevance to ultra high energy cosmic ray air showers (p. 399) |
| by Kasahara, K |
| Neural-net approach for event-direction reconstruction in ray astronomy (p. 400) |
| by Bhat, C L |
| Source searches using the CYGNUS water-Cerenkov array (p. 401) |
| by Allen, G E |
| Energetic particle activity in the heliospheree 1991-1995 (p. 401) |
| by Krimigis, S M |
| Recent extensions to the CORSIKA extensive air shower simulation program (p. 403) |
| by Knapp, J |
| Lowering threshold energy of ray telescopes - A new strategy (p. 404) |
| by Bhat, C L |
| Search for radiation above 20 TeV from supernova remnants in our galaxy (p. 405) |
| by Prosch, C |
| Quiet-time proton Fluxes in the inner heliosphere (p. 405) |
| by Zeldovich, M A |
| Simulation of Eev extensive air shower (p. 407) |
| by Attallah, R |
| An experiment to detect correlations between Cherenkov and muon lateral distributions in EAS (p. 408) |
| by Paling, S |
| Search for cosmic point sources of high energy gamma radiation above 40 TeV (p. 409) |
| by Willmer, M |
| Energetic ions near comet halley in March 1986: cometary vs interplanetary origin (p. 409) |
| by Kecskemety, K |
| Gauhati university mini-array to detect UHE cosmic rays (p. 411) |
| by Boruah, K |
| Calibration techniques for air-Cherenkov telescopes (p. 412) |
| by Biller, S D |
| Search for UHE Ray emission from discrete sources (p. 413) |
| by Blake, P R |
| An overview on measurements in high heliogaraphic latitudes: Results from EPAC on ULYSSES (p. 413) |
| by Keppler, E |
| Low frequency radio emission From large inclined showers (p. 414) |
| by Das, B |
| The university of Durham Mark 6 low energy threshold gamma-ray telescope (p. 416) |
| by Chadwick, P M |
| Search UHE Emission from the X-ray Nova GRO J1655-40 (p. 417) |
| by Clay, R W |
| Ulysses observations of high energy ions and electrons associated with CME events at high heliographic latitudes (p. 417) |
| by Anglin, J D |
| Arrival time distribution of Cerenkov photons and the elemental composition of primary cosmic rays around 10 eV (p. 418) |
| by Haustein, V |
| Enhancement of very high energy ray signals using the university of durham Mark 3A (p. 420) |
| by Chadwick, P M |
| UHE Ray astronomy with EAS-TOP (p. 421) |
| by Aglietta, M |
| Spatial gradients, energy spectra, and anisotropies of ions 30 keV at CIR shocks from 1 to 50 AU (p. 421) |
| by Decker, R B |
| Composition and energy measurement with a new method applied to the HEGRA data in the energy range of the Knee (p. 422) |
| by Lindner, A |
| MYSTIQUE - a large-area, wide-angled atmospheric Cherenkov telescope (p. 424) |
| by Bhat, C L |
| Study of UHE gamma ray sources with the GRAPES II array at Ooly (p. 425) |
| by Gupta, S K |
| Pressure and energy carried by superthermal ions during the Sep. 1991 GMIR at voyagers 1 and 2 (p. 425) |
| by Decker, R B |
| The density distribution of Cherenkov Lights produced by p and Fe simulation showers (p. 426) |
| by Luorui, S |
| Search for ultra-high energy photons from Cygnus X-3 (p. 426) |
| by Murald, Y |
| Very high resolution whipple gamma ray camera (p. 428) |
| by Sembroski, G H |
| Cosmic ray modulation by MIRs in distant heliosphere: Voyager observations (p. 429) |
| by Ness, N F |
| The shape of the atmospheric Cherenkov light images of extensive air showers (p. 430) |
| by Aglietta, M |
| A search for ultra high energy gamma-ray emission from Cygnus X-3 and Hercules X-1 (p. 430) |
| by Borione, A |
| Comparison of recurrent ion events using Ulysses HI-SCALE and EPAC and voyager LECP data (p. 431) |
| by Krupp, N |
| A CCD - based atmospheric imaging detector for SHE-UHE-EHE astroparticle physics (p. 432) |
| by Mirzoyan, R |
| Search for points sources of uhe gamma rays in 1993-1994 with the south pole air shower detector (p. 434) |
| by Beamans, J |
| Stereoscopic observation of atmospheric Cherenkov extensive air showers (p. 434) |
| by Aglietta, M |
| A search for compact sources of UHE Neutralion (p. 435) |
| by Borione, A |
| Time series analysis of low energy interplanetary charged particle fluxes and interplanetary magnetic field data (p. 435) |
| by Thomson, D J |
| Gamma-ray selection and energy measurement with the CAT imaging telescope (p. 436) |
| by Degrange, B |
| Longitudinal development of EAS using the results of Cherenkov light study (p. 438) |
| by Kalmykov, N N |
| Search for ultra high energy gamma rays from supernova Remnants (p. 439) |
| by Borione, A |
| Quiet-time â 1 MeV/nucleon fluxes as observed by the EPAC instrument on board Ulysses (p. 439) |
| by Witcombe, A |
| A new ring imaging Cherenkov telescope for measurements of light cosmic ray nuclei (p. 440) |
| by Ellithorpe, D |
| Simulations of pulses and lateral structure functions of the Cherenkov, muon and electron components in EAS at the âﾜkneeâ region of the primary energy spectrum (p. 442) |
| by Anokhina, A M |
| Search for UHE emission from supernova Remnants (p. 443) |
| by Allen, G e |
| Anisotropies of interstellar pickup protons â implications for scattering of low rigidity ( 1 to 3MV) particles (p. 443) |
| by Glöckler, G |
| A dual imaging Cherenkov experiment (DICE) for examining primary composition near the Knee of the all particle spectrum (p. 444) |
| by Boothby, K |
| Sharp difference of measured Cherenkov light quantity per shower particle by shower selection according to their size or primary energy and problem of Knee existence at E (p. 446) |
| by Yakovlev, V I |
| Search for 100 TeV Gamma Rays from southern supernova remnants with the JANZOS array (p. 447) |
| by Allen, W H |
| Ulysses radial and latitudinal gradients: Low energy proton flux measurements (p. 447) |
| by Anglin, J D |
| The CERES experiment (CERenkov energy spectrum) (p. 448) |
| by Hillas, A M |
| The EASCAMP detector at Campinas (p. 450) |
| by Birai, A R |
| High energy gamma rays above 3 TeV observed by balloon-borne JACEE emultion chambers (p. 451) |
| by Takahashi, Y |
| The periodic variation of 1 and >92 MeV proton fluxes at high latitudes (p. 451) |
| by Anglin, J D |
| Time characteristics of Cherenkov telescope âﾜHOTOVOâ (p. 452) |
| by Hristov, L L |
| Investigation of the arrival time distribution of muons with energy 5 GeV in EAS at Mountain level 9^() g/cm 2 (p. 454) |
| by Beisembaev, R U |
| A study of the diffuse gamma radiation in the energy region E =3.10 3.10 eV (p. 455) |
| by Yuldashbaev, T S |
| Effects of corotating interaction regions on Ulysses high energy particles (p. 455) |
| by Kunow, H |
| Exploitation of the themis solar plant for gamma astronomy at 20 GeV (p. 456) |
| by Paré, E |
| Arrival time distributions of muons from extensive air showers as signature of the mass composition of cosmic rays (p. 458) |
| by Volker, G |
| SAMPEX observations of corotating ion events at (p. 459) |
| by Mazur, J E |
| On the rate of UHE ray primaries (p. 459) |
| by Aglietta, M |
| Helium spectra in corotating energetic particle streams observed by EPACT on the wind spacecraft (p. 460) |
| by Mazur, J E |
| A new 127 pixel camera for cherenkov telescopes of the HEGRA array on la Palma (p. 460) |
| by Rauterberg, G |
| measurements of the ionic charge states of solar energetic particles at 15 - 70 MeV/nucleon (p. 461) |
| by Leske, R A |
| A search for anisotropy in the arrival direction of EAS by cosmic rays from discrete sources (p. 462) |
| by Chakrabarti, C |
| A search for diffuse sources of ultra high energy gamma-rays (p. 463) |
| by Borione, A |
| Cherenkov telescope calibration using muon ring images (p. 464) |
| by Rose, H J |
| Measurements of the isotopic composition of solar energetic particles (p. 465) |
| by Williams, D L |
| EAS-1000 array: 1995 Year Status (p. 466) |
| by Ameev, S S |
| The source plasma of solar energetic particles in gradual events (p. 466) |
| by Boberg, P R |
| Loss processes in the accretion column accelerator of Hercules X-1 (p. 467) |
| by Johnson, P A |
| Parameter optimization and calculated performance for the THEMISTOCLE multi-mirror Cherenkov technique (p. 468) |
| by Eschstruth, P T |
| The wide angle air-Cherenkov detector AIROBICC at la Palma (p. 470) |
| by Arqueros, F |
| Charge states of heavy solar energetic particles: Observations with the HILT sensor on SAMPEX (p. 470) |
| by Oetliker, M |
| Search for radiation from the SNR G78.2+2.1:A test of the SNR Theory of cosmic ray Origin (p. 471) |
| by Prosch, C |
| The high resolution fast imaging device of the G.A.M.T. experiment (p. 472) |
| by Auriemma, G |
| Charge state measurements of solar energetic Particles observed with SAMPEX (p. 474) |
| by Mason, G M |
| Status of the HEGRA experiment at La Palma (p. 474) |
| by Fonseca, V |
| SAMPEX studies of anomalous cosmic ray contributions to hydrogen and helium at 1 AU (p. 475) |
| by Cummings, J R |
| Observations of teV Gamma rays from supernova remnants (p. 475) |
| by Lessard, R W |
| SAMPEX studies of anomalous cosmic ray from 1992 to 1995 (p. 476) |
| by Cummings, J R |
| CANGAROO stereo observations of TeV gamma ray sources (p. 476) |
| by Thornton, G J |
| Studies of anomalous cosmic rays using the geomagnetic field (p. 477) |
| by Mewaldt, R A |
| An improved search for gamma radiation from cosmic point sources using a hadron separation procedure on the AIROBICC 92/93 data (p. 479) |
| by Moralejo, A |
| Central receiver Cherenkov Array: On-site test results at solar two (p. 480) |
| by Ong R A |
| Trapped Low-energy heavy ion results from LDEF (p. 481) |
| by Kleis, T |
| Status of the experiment ANI the first stage - installation âﾜGammaâ (p. 482) |
| by Arzumanian, S A |
| The source of TeV gamma-rays in Cen X3 (p. 483) |
| by Raubenheimer, B C |
| A Cherenkov array at Soudan (p. 484) |
| by Border, P |
| Cosmos results on the altitude dependence of geomagnetically trapped anomalous cosmic rays (p. 485) |
| by Tylka, A J |
| âﾜMuon eyeâ array, its characteristics and advantages (p. 486) |
| by Dumora, D |
| Observation of 2CG006-00/CGRO J1758-23 at TeV energies (p. 487) |
| by Mori, M |
| Sensivity of extensive air shower array to gamma ray flux (p. 488) |
| by Badran, H M |
| Charge states of anomalous cosmic rays: SAMPEX Observations (p. 489) |
| by Klecker, B |
| Study of primary cosmic ray energy spectrum with a compact electron detector array (GRAPES III experiment at Ooty) (p. 490) |
| by Sivaprasad, K |
| Camera Obscura network-array for registration of EAS Cerenkov radiation (p. 491) |
| by Garipov, G K |
| Observations of Markarian 421 by the Whipple observatory collaboration (p. 491) |
| by Lamb, R C |
| A digital trigger for the FADC Electronics system for the HiRes detector (p. 492) |
| by Boyer, J |
| Ionization states of anomalous cosmic rays inside magnetosphere (p. 493) |
| by Yadav, J S |
| A method for separation of y and hadron initiated air showers with angle integrating Cerenkov arrays (p. 495) |
| by Arqueros, F |
| A search for high energy radiation from mkn 421 using the imaging Cherenkov telescopes of the HEGRA collaboration (p. 495) |
| by Petry, D |
| An ideal detector for UHE ray astronomy (p. 496) |
| by Chernyaev, A B |
| Elemental composition of the anomalous cosmic ray component (p. 497) |
| by Cummings, A C |
| Determination of the depth of maximum development and primary energy of cosmic ray showers with AIROBICC (p. 499) |
| by Cortina, J |
| The high energy gamma ray spectrum of Mrk421 (p. 499) |
| by Protheroe, R J |
| Preliminary analysis of monocular HiRes prototype data (p. 500) |
| by Bird, D J |
| A search for molecular ions in the anomalous cosmic rays (p. 501) |
| by Looper, M D |
| Photoproduction in gamma initiated showers (p. 503) |
| by Krys, E |
| A search for ultra-High energy gamma rays from active galactic nuclei with CASA-MIA (p. 503) |
| by Borione, A |
| The high resolution Fly's eye project (p. 504) |
| by Bird, D J |
| Anomalous cosmic ray oxygen ( 2.5 MeV/nucl) at high southern heliolatitudes on Ulysses (p. 505) |
| by MacLennan, C G |
| Single-particle detection efficiency and e rejection power of lst stacks in the Palermo-Leeds-Napoli Track time experiment (p. 507) |
| by Catalano, O |
| An upper limit to the IR Background from observation of TeV gamma-rays (p. 507) |
| by Biller, S D |
| Pointing accuracy of a full coverage RPC's carpet operating at high altitude (p. 508) |
| by Casolino, M |
| Clusters of muons underground : a new tool for cosmic ray studies(p. 508) |
| by Battistoni, G |
| Temporal development of the heliospheric magnetic field topology as confirmed by eclipse observations of the solar corona streamers (p. 509) |
| by Sykora, J |
| Pair halos around nonthermal extragalactic sources. Possible cosmological probes (p. 511) |
| by Aharonian, F |
| Observation of penetrating muons through mountain (p. 512) |
| by Aoki, T |
| Recent Upgrades to CASA-MIA (p. 512) |
| by Borione, A |
| Persistent larger IMF spiral north of the heliospheric current sheet than south of it (p. 513) |
| by Sabbah, I |
| Implications of modified AGN Spectra due to absorption by infrared photons (p. 515) |
| by Biller, S D |
| Particle fluxes in the atmosphere and geomagnetic effects (p. 516) |
| by Lipari, P |
| Gamma-ray bursts: Detection and distance estimates with Milagro (p. 516) |
| by Allen, G E |
| Year cosmic ray variations (p. 517) |
| by Chebakova, E A |
| Reverberation mapping of central regions of AGN using high-energy ray observations (p. 519) |
| by Böttcher, M |
| Delayed muons and their relation to primary cosmic rays (p. 520) |
| by Wentz, J |
| Feasibility study of water Cherenkov detector at Mt. Norikura (p. 520) |
| by Kajino, F |
| Year variation N-S asymmetry and cosmic ray gradient change (p. 522) |
| by Kolomeets, E V |
| Proton interactions in AGN Jets (p. 523) |
| by Johnson, P A |
| The analysis of the PCR nucleon energy spectrum and charm production cross-section as observed in MSU muon experiment (p. 524) |
| by Ilina, N P |
| Gamma-ray production in astrophysical jets (p. 524) |
| by Protheroe, R J |
| Water Cerenkov detector for a detection of gamma-ray bursts at high altitude (p. 524) |
| by Kajino, F |
| Simulation of long term modulation in nonstationary solar activity conditions (p. 526) |
| by Kryakunova, O N |
| Study of primary interactions with multiple muons events in MACRO (p. 528) |
| by Battistoni, G |
| The expected flux of TeV photons from plerions (p. 528) |
| by De Jager, O c |
| The present status of the new Tibet air shower experiment (p. 528) |
| by Amenomori, M |
| Role of LDE-Type flares in the GCR Modulation (1969-1972) (p. 530) |
| by Antalova, A |
| The prompt muon component in very high energy cosmic ray showers (p. 532) |
| by Battistoni, G |
| Inverse problem approach to gamma ray propagation (p. 532) |
| by Entel M B |
| Daily values of the solar SXR background and galactic cosmic ray modulation (1968-1972) (p. 534) |
| by Antalova, A |
| Analysis of muon events recorded with the NT-36 detector in Lake Baikal (p. 536) |
| by Belolaptikov, I A |
| Propagation of ultra high energy photons through the intergalactic medium (p. 536) |
| by Lee, S |
| Primary composition study using a new parameter for a constant efficiency selection of EAS at Mountain Altitudes (p. 536) |
| by Batovsky, S A |
| Galactic cosmic ray intensity at earth an polar coronal hole area (p. 538) |
| by Bravo, S |
| MACRO absolute muon flux measurement: comparison with Monte Carlo predictions (p. 540) |
| by Bussino, S |
| Observation of AGN at TeV energies by project CANGAROO (p. 540) |
| by Kifume, T |
| Selection of EAS with constant energy in the Tibet Experiment (p. 540) |
| by Dumora, D |
| Long-term cosmic ray variations and their relation with solar activity parameters (p. 542) |
| by Belov, A V |
| Comparison of the LVD single muon angular distribution with simulated data (p. 544) |
| by De Silva, A |
| Gamma-ray observations in moonlight with the whipple atmospheric Cherenkov Hybrid camera (p. 544) |
| by Chantell, M |
| Detection efficiency of a small size showers by a full coverage RPCs carpet (p. 544) |
| by D'Ettorre-Piazzoli, B |
| Power spectrum of cosmic rays in the frequency range (3x10 2x10 Hz) (p. 546) |
| by Otaola, J |
| Atmospheric single muon flux measured over five decades of intensity by LVD at Gran Sasso laboratory (p. 548) |
| by Giusti, P |
| Methods to reconstruct the energy of gamma ray atmospheric showers in the Themistocle experiment (p. 548) |
| by Espigat, P |
| The HiRes2 prototype and coincident measurements with HiRes1 (p. 548) |
| by Bird, D J |
| The energy hysteresis of the galactic cosmic ray intensity in 1988-1993 (p. 550) |
| by Svirzhevsky, N S |
| A study of single muon I (O, X) structure observed in the LVD particle astrophysics experiment (p. 552) |
| by Hafen, E S |
| Multi-spectral band observations on gamma-ray sources (p. 552) |
| by Kaul, R K |
| Reconstruction techniques of monocular HiRes data with a FADC electronics System (p. 552) |
| by Boyer, J |
| Present status of the recovery phase of cosmic ray eleven year modulation (p. 554) |
| by Ahluwalia, H S |
| The features of the long-period modulation of galactic cosmic rays (p. 555) |
| by Alania, M V |
| Study of primary cosmic ray composition using a very large area muon detector (GRAPES III experiment at Ooty (p. 556) |
| by Kawakami, S |
| Ability of cosmic ray rejection based on simultaneous registration of the integral Cherenkov light intensities from air showers by multitelescope system used in VHE ray (p. 556) |
| by Konopelko, A K |
| An analysis of EAS with energies above the GZK cit-off (p. 556) |
| by Dedenko, L G |
| Power index of pion and kaon spectrum in the atmosphere obtained with LVD at Gran Sasso (p. 557) |
| by Kudryavtsev, V A |
| The simulation of galactic cosmic rays heliolatitudinal modulation (p. 559) |
| by Alania, M V |
| The use of a UV camera in the atmospheric Cherenkov technique (p. 560) |
| by Chantell, M C |
| Atmospheric monitoring for fluorescence detector experiments (p. 560) |
| by Bird D J |
| 27-day variation of galactic cosmic rays (p. 560) |
| by Sabbah, I |
| Detection of events with muon multiplicity N 1500 at the Baksan underground scintillation telescope (p. 561) |
| by Bakatanov, V N |
| Pion Eye a method of measuring the chemical composition of Auger radiation with high resolution up to and beyond 10 eV/nucleus (p. 564) |
| by Linsley, J |
| Images of atmospheric Cherenkov light showers for TeV energies (p. 564) |
| by Aliaga, Z |
| Amplitude of the 27-Day cosmic ray variation in 19-21 solar cycles (p. 564) |
| by Vernova, E S |
| High energy muon spectra at zenith angles 0 and 89 (p. 565) |
| by Bhattacharya, D P |
| The MIR-SPECTR gamma-astronomy experiment (p. 567) |
| by Kudryavtsev, M I |
| Relative elemental abundances of Ne to Ni in the primary cosmic rays over Alice Springs and the predicted source spectrum (p. 568) |
| by Bhattacharya, D P |
| Recurrent changes in cosmic ray neutron component (1958-1992) (p. 568) |
| by Levitin, A E |
| Low and high energy muons in extensive air showers of size 10 to 10 particles (p. 569) |
| by Chakrabarti, C |
| A prompt report on the first Russo-Japanese joint balloon experiment (p. 571) |
| by Apanasenko, A V |
| Some preliminary results of the ultra heavy cosmic ray elemental abundances measured on the ultra heavy cosmic ray experiment (UHCRE) (p. 572) |
| by Domingo, C |
| Long-term changes in galactic cosmic ray variation caused by the solar rotation (p. 572) |
| by Bazilevskaya, G A |
| High energy muon production in iron generated EAS for superposition and fragmentation models (p. 573) |
| by Attallah, R |
| A balloon borne electron telescope with scintillating fibers (p. 575) |
| by Torii, S |
| Voyager measurements of the isotopic composition of Sc, Ti, V, Cr, Mn and Fe Nuclei (p. 576) |
| by Lukasiak, A |
| 27-Day waves in the cosmic ray north-south anisotropy (p. 576) |
| by Swinson, D B, |
| Study of interactions of TeV muons by means of underground cosmic ray experiments (p. 577) |
| by Battistoni, G |
| Performance of BESS detector (p. 579) |
| by Nozaki, M |
| Status report on HIIS observations of ultraheavy galactic cosmic rays (p. 580) |
| by Tylka, A J |
| Long-term variations of cosmic Ray north-south anisoptropy in 70-and 80-th years (p. 580) |
| by Belov, A V |
| Search for anisotropies in deep underground muons (p. 581) |
| by Marshak, M L |
| The Ultraheavy composition detector of the trek experiment (p. 581) |
| by Westphal, A J |
| A search for cosmic point sources of muons and for seasonal variations in the underground muon flux with the MACRO detector (p. 582) |
| by Ahlen, S P |
| Detecting cosmic ray iron using balloon-borne air Cherenkov detectors (p. 583) |
| by Seckel, D |
| Numerical simulations of the cosmic-ray diurnal anisotropy (p. 584) |
| by Sabbah, I |
| Measurement of the cosmic ray muon spectrum and charge ratio in the atmosphere from ground level to balloon altitudes (p. 585) |
| by Basini, G |
| The energy dependence of lithium to carbon abundance ratio in galactic cosmic rays (p. 585) |
| by Evenson, P |
| Results from the flight of BUGS-4 (p. 587) |
| by Smith, A E |
| The North-south asymmetry of cosmic rays as dependence from a sectorial structure of the interplanetary magnetic field (p. 588) |
| by Gorchakov, E V |
| Monte Carlo calculations of atmospheric electrons compared with data from HEAT (p. 589) |
| by De Nolfo, G |
| Ulysses high energy telescope elemental measurements: secondary to primary ratios of galactic cosmic rays (p. 589) |
| by Duvernois, M A |
| The magnetic spectrometer PAMELA for the study of cosmic antimatter in space (p. 591) |
| by Adriani, O |
| Cosmic-ray diurnal variation during the 1964-1992 epoch (p. 592) |
| by Borello Filisetti, O |
| Further results from the LDEF ultra heavy cosmic ray experiment (p. 593) |
| by Thompson, A |
| Measurement of the cosmic ray induced muon flux through the atmosphere using IMAX (p. 593) |
| by Krizmanic, J F |
| Ratio of sub-iron to iron ion abundances of low energy galactic cosmic rays (p. 594) |
| by Vahia, M N |
| Maximum energy Auger air shower satellite (MASS) for observing cosmic rays in the energy region 10 eV (p. 595) |
| by Takahashi, Y |
| Variation of diurnal anisotropy during Minimum of solar activity cycles 20 & 21 (p. 596) |
| by Sharma, N K |
| Study of the radiative interactions of 300 GeV muons in a high resolution calorimeter (p. 597) |
| by Battistoni, G |
| The deuterium cosmic ray intensity from balloon measurement in energy range 0.8-1.8 (p. 598) |
| by Bogomolov, E A |
| Flight performance of the HEAT rigidity spectrometer (p. 599) |
| by Tomasch, A D |
| Cosmic ray solar diurnal variations gradients and the interplanetary magnetic field (p. 599) |
| by El-Borie, M A |
| Multiple interactions of muon energy spectrum deep underground (p. 601) |
| by Castagnoli, C |
| The Ulysses cosmic ray isotope experiment: isotopic abundances of Fe and Ni from high resolution measurements (p. 602) |
| by Connell, J J |
| Flight performance and electron-hadron separation of the HEAT - e experiment (p. 603) |
| by Torbet, E |
| Dependence of the solar diurnal variations upon the magnetic polarity of the heliosphere (p. 603) |
| by El-Borie, M A |
| Muon transport in a random medium (p. 605) |
| by Lagutin, A A |
| The isotopic composition of anomalous and galactic cosmic rays from SAMPEX (p. 606) |
| by Leske, R A |
| A satellite born charged particles telescope for the study of cosmic ray nuclei (p. 607) |
| by Barbiellini, G |
| The parallel mean-free path of galactic cosmic rays at 1 AU (p. 607) |
| by Hall, D L |
| Helium 3 local interstellar spectra derived by demodulating measured spectra (p. 610) |
| by O'Neil, P M |
| Balloon flight tests of a Gas-ionization chamber-based isotope spectrometer (p. 611) |
| by Wiedenbeck, M E |
| Asymmetric heliospheric modulation of a galactic anisotropy (p. 611) |
| by Hall, D L |
| Search for point sources of deep underground muons (p. 613) |
| by Marshak, M L |
| Muons from the direction of cygnus X-3 1992-1994 (p. 614) |
| by Tsuji, S |
| Cosmic ray hydrogen isotopes from 0,2 to 3.0 GeV/nucleon (p. 614) |
| by Davis, A J |
| Antarctic balloon flights for JACEE (p. 615) |
| by Wilkes, R J |
| Observation of the first-three harmonics of cosmic-ray daily intensity variations and the magnetic polarity of the heliosphere (p. 615) |
| by Munakata, Y |
| Phase analyses of muons from the direction of Cygnus X-3 at large zenith angles: 1992 - 1994 (p. 618) |
| by Tsuji, S |
| The cosmic ray He He ratio from 0.2 to 3.6 GeV/nucleon (p. 618) |
| by Reimer, O |
| Long flying component and incorrect measurements of proton energy spectrum by shallow arrays at E>10 TeV (p. 619) |
| by Yakovlev, V L |
| Long term behaviour of semidiurnal variations of cosmic ray intensity (p. 619) |
| by El-Borie, M A |
| Muons from the direction of Cygnus X â 3 during july 1990-december 1991 radio flares (p. 622) |
| by Tsutsui Y |
| Interpretation of the helium isotope ratios measured by IMAX (p. 622) |
| by Davis, A J |
| A telemetry frame sync board for use in balloon payloads (p. 623) |
| by Christian, E R |
| Tri-diurnal variation in cosmic ray intensity on quiet days during solar cycles 21-22 (p. 623) |
| by Kumar, S |
| Estimation of integral muon spectrum from point source photon spectrum (p. 626) |
| by Bhattacharya, D P |
| Cosmic ray H and He isotopes in the outer heliosphere in 1994 (p. 626) |
| by Seo, E S |
| The space physics data system - cosmic and heliospheric nodes (p. 627) |
| by Garrard, T L |
| Diurnal variations underground since 1959 (p. 627) |
| by Swinson, D B |
| Muon range fluctuations in Rock (p. 630) |
| by Makarov, V V |
| Measurements of cosmic ray helium during the 1991 solar maximum (p. 630) |
| by Wefel, J P |
| Effects of galactic cosmic ray modulation in the heliosphere (p. 631) |
| by Krymsky, G F |
| Gamma-telescope with crystal converter (p. 631) |
| by Khablo, V A |
| The atmospheric background pf protons and deuterons measured at 5 cm2 (p. 634) |
| by Wefel, J P |
| Sidereal variations at high energies - observations at poatina (p. 635) |
| by Fenton, K B |
| Performance of the BUGS IV spherical drift chamber (p. 637) |
| by Petruzzo, J J |
| The HE muon and neutrino fluxes from measurements of horizontal air showers at EAS-TOP (p. 638) |
| by Aglietta, M |
| Isotopic composition of iron-group elements from the trek experiment (p. 638) |
| by Westphal, A J |
| Two hemisphere observations of the north-south sidereal asymmetry at 1TeV (p. 639) |
| by Munakata, K |
| Direct coulomb Electron pairs for energy measurement - design consideration (p. 641) |
| by Derrickson, J H |
| Interactions of the UHE cosmic ray neutrinos with the cosmological neutrino background (p. 642) |
| by Sivaram, C |
| Sanriku Balloon experiment for cosmic heavy primary observation (p. 642) |
| by Dol, T |
| Sidereal diurnal variations observed by the two hemisphere network of surface level muon telescopes (p. 643) |
| by Munakata, K |
| Application of the image calorimeter in the high energy gamma astronomy (p. 645) |
| by Carlson, Per J |
| The galactic cosmic ray all-particles spectrum, preliminary results from the TIC experiment (p. 646) |
| by Adams, J H |
| Muons of extra high energy horizontal EAS in geomagnetic field and nucleonic astronomy (p. 646) |
| by Pavluchenko, V P |
| Long term change in the sidereal diurnal variation observed by the Misato shallow underground muon telescope (p. 647) |
| by Munakata, K |
| Measurement of cosmic ray H and He spectra in a balloon bome experiment with a superconducting solenoid spectrometer (p. 648) |
| by Seo, ES |
| Observation of sidereal anisotropy of cosmic rays at 1 TV (p. 648) |
| by Mori, S |
| A study of a high pressure microstrip gas chamber (p. 649) |
| by Ortuno-Prados, F |
| Characterisation of the energy spectrum of Ni from stellar collapses with the detector (p. 650) |
| by Chinellato, J A |
| The relative fluxes of protons and helium nuclei up to 100 GeV/n (p. 652) |
| by Swordy, S P |
| Cosmic-ray sidereal daily variation, showing of the coexistence of the galactic and heliomagnetotail-In anisotropies (p. 652) |
| by Nagashima, K |
| The ACE-CRIS scintillating fiber hodoscope: A prototype calibration at the MSU NSCL (p. 653) |
| by Hink, P L |
| A search for radiative neutrino decay from supermovae (p. 654) |
| by Miller, S |
| Cosmic ray individual element spectra: Prediction and data (p. 656) |
| by Wiebel-Sooth, B |
| Cosmic-ray excess flux from heliomagnetotail (p. 656) |
| by Nagashima, K |
| The CAPRICE RICH detector (p. 657) |
| by Barbiellini, G |
| A system to search for supernova bursts with the AMANDA detector (p. 658) |
| by Wischnewski, R |
| To the problem on the primary nucleon spectrum (p. 660) |
| by Apanasenko, A V |
| The cosmic ray convection-diffusion anisotropy according to ground and underground observations in 1965-1990 (p. 660) |
| by Ahluwalia, H S |
| Analysis of underground events recorded in the Lvd experiment at Gran Sasso correlated with ray bursts (p. 662) |
| by Galleotti, P |
| Study of the primary composition from the Ne data at EAS-TOP (p. 664) |
| by Alessandro, B |
| Drift anisotropy and transverse gradients of cosmic rays in the interplanetary space (p. 664) |
| by Dorman, L I |
| Instrumental background in high pressure X-ray gas detectors (p. 665) |
| by Feroci, M |
| Neutral current interactions of high energy neutrinos with matter of the sun and earth (p. 666) |
| by Bugaev, E V |
| Muons in extensive air showers and the cosmic-ray composition near the Knee (p. 668) |
| by Bernlöhr, K |
| The important parameters of solar wind and IMF for cosmic ray anisotropy and their dependence on heliolatitude and solar activity (p. 668) |
| by Dorman, L I |
| Status of the GILDA project for the 30 Mev- 100 GeV high energy gamma ray astrophysics (p. 669) |
| by Morselli, A |
| Possible parameterizati9on of parton distributions at small-x and neutrino-nucleon total cross section (p. 670) |
| by Butkevich, A V |
| Higher harmonics of cosmic ray solar diurnal variation. 1. persistence analysis (p. 672) |
| by Fikani, M M |
| Re-examination on primary cosmic ray composition above 10 eV (p. 672) |
| by Dai, H Y |
| Higher harmonics of cosmic ray solar diurnal variation. 2. amplitude dependence on asymptotic latitude of viewing (p. 673) |
| by Fikani, M M |
| The ACE-CRIS scintillating optical fiber trajectory (SOFT) detector (p. 673) |
| by Klarmann, J |
| Higher harmonics of cosmic ray solar diurnal variation. 3. dependence on primary rigidity (p. 674) |
| by Fikani, M M |
| The cxlculated rate of cosmogenic isotopes production by cosmic ray muons inside bulk water detectors (p. 674) |
| by Dedenko, L G |
| On correlation between Tilt of heliospheric current sheet and transverse cosmic ray particle density gradient (p. 675) |
| by Ygbuhay, R C |
| Composition studies with the CASA-MIA detector (p. 676) |
| by Borione, A |
| Modulation of high energy cosmic rays throughout the solar activity and the magnetic cycles (p. 676) |
| by Bennett, E |
| Energy estimate for very high energy cascade by core-size method in the jacee emulsion chamber (p. 677) |
| by Takahashi, Y |
| The neutrino cross section and atmospheric Neutrinos (p. 678) |
| by Lipari, P |
| Chemical composition of primary cosmic rays with energies above 100 Tev observed at Mt. Chacaltaya (p. 680) |
| by Kakimoto, F |
| 3-D Distribution of cosmic rays in the outer heliosphere (p. 680) |
| by Kota, J |
| Primary mass composition around the âﾜkneeâ in the primary spectrum (p. 681) |
| by Kempa, J |
| The trans-iron galactic element recorder (TIGER) experiment (p. 681) |
| by Lawrence, D J |
| On the high-energy limit of cosmic-ray modulation and anisotropies (p. 684) |
| by Kota, J |
| A thin electronic calorimeter for galactic cosmic ray spectral measurements (p. 685) |
| by Adams, J H |
| Measurement of the upward-going muon flux with the baksan underground telescope (p. 686) |
| by Boliev, M M |
| On the 2D and 3D cosmic ray transport equations (p. 688) |
| by Kalinin, M S |
| Estimate of the primary cosmic ray composition from a multi-parametric fit of MACRO multimuon events (p. 689) |
| by Palamara, O |
| Very heavy nuclei charge detection in fuji ET-7B nuclear emulsion in a balloon-borne (p. 689) |
| by Basu, B |
| Measurement of the ratio as a function of depth in the atmosphere (p. 690) |
| by Schneider, E |
| The influence of the nonsteady solar magnetic fields on the galactic cosmic rays (p. 692) |
| by Kalinin, M S |
| The galactic cosmic ray - current sheet relationship during last four solar cycles (p. 693) |
| by Korolkov, D N |
| A study of the coarse chemical composition of cosmic radiation between 300 and 1000 TeV (p. 693) |
| by Plaga, R |
| A new type of emulsion chamber for RUNJOB-program (1) â chamber-designing and data processing (p. 693) |
| by Apanasenko, A V |
| An improved calculation of the atmospheric neutrino flux in the GeV range (p. 694) |
| by Gaisser, T K |
| The diffusion tensor throughout the heliosphere (p. 694) |
| by Bieber, J W |
| Expectations for cosmic ray composition changes in the region 10**14 to 10**16 eV (p. 697) |
| by Swordy, S P |
| A new type of emulsion chamber for runjob-program energy determination (p. 697) |
| by Apanasenko, A V |
| The mathematical treatment of the passage of neutrinos through the universe with the fractal structure (p. 698) |
| by Uchaikin, V V |
| Heliospheric propagation of galactic cosmic rays: quasilinear theory versus hard-sphere scattering (p. 698) |
| by Hattingh, M |
| Study of primary cosmic ray composition at 10**14 - 10**15 eV: results from GRAPES II array at Ooty (p. 701) |
| by Tonwar, S C |
| A new detection technique for ZeV cosmic rays (p. 701) |
| by Kieda, D B |
| Study of primary cosmic ray composition at 10**13 - 10**14 eV with the GRAPES III array at Ooty (p. 702) |
| by Ito, N |
| Comparison of neutrino flux calculations (p. 702) |
| by Gaisser, T K |
| Phase lag effects in cosmic ray modulation (p. 702) |
| by Steenberg, C D |
| Composition and energy spectrum of cosmic rays above 30 TeV (p. 703) |
| by Yoshi, H |
| Gamma-radiation of the high energy and GAMMA-400 Project (p. 705) |
| by Fradkin, M I |
| Atmospheric neutrino oscillations in a scheme with mixing between three generations and long baseline experiments (p. 706) |
| by Bilensky, S M |
| Cosmic-ray electron modulation using current knowledge of the heliosphere (p. 706) |
| by Haasbroek, L J |
| Energy spectra and elemental composition of nuclei above 100 TeV from a series of the JACEE balloon Flight (p. 707) |
| by Asakimori, K |
| Prototype studies by the Haverah park group for the giant air shower project (p. 709) |
| by Beaman, J |
| Calculation of atmospheric neutrino fluxes in energy range of 1-3000 GeV (p. 710) |
| by Honda, M |
| Study of the primary cosmic ray composition in the PeV region with EAS-TOP and Macro (p. 710) |
| by Vallania, P |
| Cosmic ray ion identification using multistrip silicon dE/dx detectors (p. 710) |
| by Menichelli, M |
| The time-dependent Recovery after the large cosmic-ray decrease in 1991 (p. 710) |
| by Haasbroek L J |
| Study of the neutrino oscillation using atmospheric neutrinos (p. 714) |
| by Honda, M |
| Performance of the transition radiation detector flown on the NMSU/WIZARD TS93 balloon-borne instrument (p. 714) |
| by Aversa, F |
| Heliospheric cosmic ray distributions: a tool for probing the solar wind termination (p. 714) |
| by Fichtner, H |
| Underground-surface coincidences at Soudan (p. 714) |
| by Border, P |
| Cosmic rays shower maximum in the 0.01 to 1 EeV region - results from HiRes/FE2 coincident data (p. 718) |
| by Bird, D J |
| Preliminary Results from IMB3 muon/electron identification tests at KEK (p. 718) |
| by Bratton, C B |
| Advanced thin ionization calorimeter (ATIC) (p. 718) |
| by Isbert, J |
| The maximum energy of anomalous cosmic rays (p. 718) |
| by Jokipii, J R |
| On the chemical composition of primary cosmic rays in the energy region E = (40 - 100) TeV/n (BAKSAN experiment) (p. 720) |
| by Bakatanov, V N |
| Search for astro[physical sources of neutrinos oscillations using the baksan data (p. 722) |
| by Boliev, M M |
| Study of cosmic ray nuclei detection by an image calorimeter (p. 722) |
| by Carlson, Per J |
| A transport model for the diffusive shock acceleration and modulation of the anomalous component in the heliosphere (p. 722) |
| by Le Roux, J A |
| The energy spectrum of primary cosmic rays by the data of tunka Cherenkov array (p. 724) |
| by Bryanski, S V |
| Absolute measurement of the muon and electron neutrino flux with the Frejus experiment (p. 726) |
| by Rhode, W |
| Ion identification method using E-E measurements (p. 726) |
| by Bronchalo, E |
| The dynamic relevance of the heliospheric magnetic field accordind to a spherically-symmetric particle hydromagnetic model (p. 726) |
| by Le Roux, J A |
| Cosmic ray proton and helium spectra - combined JACEE results (p. 728) |
| by Cherry, M L |
| Statistical studies of the pressure of interstellar pick-up ions: implications for the outer heliosphere (p. 730) |
| by Fisk, L A |
| Upward-going muons in macro (p. 730) |
| by Di Credico, A |
| Use of neutral network techniques to identify cosmic ray electrons and positrons during the 1993 balloon flight of the NMSU/Wizard-TS93 instrument (p. 730) |
| by Bellotti, R |
| Continuous production of anomalous cosmic rays forming a dissipative shock precursor (p. 731) |
| by Chalov, S V |
| A measurement of the EAS differential size spectrum for 10 >Ne< 10 and of the absorption of EAS in the atmosphere (p. 732) |
| by Chiavassa, A |
| Neutrino-induced single-muon flux measured by LVD at Gran Sasso (p. 734) |
| by Sartorelli, G |
| Computer network-based data acquisition and control system for TACTIC (p. 734) |
| by Koul, R |
| A numerical model for the anomalous component of cosmic rays (p. 735) |
| by Steenkamp, R |
| Primary cosmic rays at the âﾜKneeâ energy region observed with the Tibet air shower array (p. 736) |
| by Amenomori, M |
| Variation of the atmospheric neutrino integral fluxex from up and down earth's hemispheres (p. 738) |
| by Kolomeets, E V |
| Front-end instrumentation of TACTIC imaging ray telescope (p. 738) |
| by Rannot, R C |
| Model calculations on anomalous hydrogen (p. 739) |
| by Steenberg, C D |
| The cosmic ray energy spectrum above 1X10 eV determined by AGASA (p. 740) |
| by Doi, T |
| The lake BAIKAL neutrino project : status report(p. 742) |
| by Belolaptikov, I A |
| Optimizing the non-linear gamma-ray domain in VHE gamma-ray astronomy using a neural network classifier (p. 742) |
| by Chilingarian, A A |
| The effect of drifts on the calculation of the spectra of anomalous cosmic ray during solar minimum conditions (p. 743) |
| by Reinecke, J P |
| The energy spectrum of cosmic rays with the CASA-MIA air shower array (p. 744) |
| by Borione, A |
| KM3 as a detector of atmospheric muons (p. 746) |
| by Kokoulin, R P |
| The use of GPS clocks for high relative timing accuracy between HiRes sites (p. 746) |
| by Bird, D J |
| the cosmic ray state of the heliosphere during solar minimum (p. 747) |
| by Reinecke, J P |
| The primary cosmic ray spectrum at 2X10 -2X10 eV and its peculiarity above 10 eV according to Tien-Shan data (p. 748) |
| by Nesterova, N M |
| Possible signatures of a large extragalactic proton flux at HiRes (p. 750) |
| by Boyer, J |
| A flash ADC electronics system for the HiRes Detector (p. 750) |
| by Boyer, J |
| The modeling study of cosmic ray long-period modulation (p. 751) |
| by Alania, M V |
| results from an Antarctic balloon flight (p. 752) |
| by Olson, E D |
| Evolution of the electron/proton ratios between 1 and 7 GV measured at Ulysses, as a function of time and latitude (p. 752) |
| by Ferrando, P |
| Flux of high-energy neutrino-induced muons from active galactic nuclei (p. 754) |
| by Minorikawa, Y |
| A genetic algorithm for optimizing TeV gamma-ray selection (p. 754) |
| by Lang, M J |
| The primary spectrum of cosmic rays of energy above 10 eV by the Yakutsk EAS array data (p. 756) |
| by Afanasiev, B V |
| Latitudinal effects of galactic cosmic rays observed onboard the Ulysses spacecraft (p. 756) |
| by Paizis, C |
| Status and capabilities of AMANDA-94 (p. 758) |
| by Mock, P C |
| Calibration studies of the FADC electronics system for the HiRes detector (p. 758) |
| by Boyer, J |
| Multi-component observations of 10eV EAS with the CASA-MIA and HiRes detectors (p. 760) |
| by Bird, D J |
| The latitudinal gradient of anomalous cosmic rays: Ulysses observations (p. 760) |
| by Trattner, K J |
| Search for neutrinos from collapsing stars with the LVD experiment in Gran Sasso (p. 762) |
| by Galleotti, P |
| Nucleon modulation from the ULYSSES rapid latitude scan: COSPIN/KET results (p. 764) |
| by Heber, B |
| Monte Carlo study of DUMAND Three-string array (p. 766) |
| by Okada, A |
| A data acquisition system for TeV stereo imaging telescopes (p. 766) |
| by Rose, H J |
| SPASE - AMANDA coincidences at the south pole (p. 768) |
| by Miller, T C |
| Long-term cosmic-ray modulation along the Ulysses trajectory: a numerical simulation (p. 768) |
| by Haasbroek, L J |
| Variation of water parameters at the site of the Baikal experiment and their effect on the detector performance (p. 770) |
| by Belolaptikov, I A |
| Neural networks for hadron-separation with the HEGRA Geiger towers (p. 770) |
| by Westerhoff, S |
| The energy spectrum and the mass composition of the primary cosmic rays around the Knee (p. 772) |
| by Kristiansen, G B |
| Radial density gradients of galactic cosmic rays from 1973 to 1995 (p. 772) |
| by Fujii, Z |
| Possibility to select neutrino-induced muons in Cherenkov water detector on the earth's surface (p. 773) |
| by Aynutdinov, V M |
| Cosmic rays as energy sources for chemical evolution (p. 774) |
| by Saitô, T |
| Energy spectrum of primary cosmic rays at energies 100-200 TeV measured with Thian - Shan atmospheric Cerenkov telescope (TACT) (p. 776) |
| by Antonov, R A |
| Properties of step decreases observed in solar cycle 22 (p. 776) |
| by Fujii, Z |
| Optical properties of south pole ice for neutrino astrophysics (p. 777) |
| by Price, P B |
| The arrival direction of EAS above 10 eV determined with Kinki array at sea level (p. 780) |
| by Chikawa, M |
| The initial cosmic ray recovery phase of solar cycle 22 (p. 780) |
| by McDonald, F B |
| Search for high energetic muon neutrinos with the Frejus detector (p. 781) |
| by Rhode, W |
| Solid hydrogen as dark matter? (p. 782) |
| by Stephen White, R |
| Galactic anisotropy above 1 EeV (p. 784) |
| by Smith, A G |
| Radial and latitudinal cosmic ray intensity gradients in the outer heliosphere (p. 784) |
| by McDonald, F B |
| Possibilities of construction and development of big underwater neutrino telescope on Lake Baikal (p. 785) |
| by Bezrukov, L B |
| One possible mechanism of electromagnetic radiation arising from intermediate boundary between conducting ans superconducting media within pulsar (p. 786) |
| by Ahmedov, B J |
| CASA-MIA observation of sun and Moon shadows (p. 788) |
| by Borione, A |
| Studies of anomalous cosmic ray hydrogen in the outer heliosphere (p. 788) |
| by McDonald, F B |
| Separation of upward moving muons in the Baikal underwater telescope (p. 789) |
| by Belolaptikov, I A |
| Triplet pair production in electron-photon cascading in a soft photon field (p. 790) |
| by Anguelov, V |
| EAS-sideral anisotropies as seen by power spectrum techniques (p. 792) |
| by Martinic, N J |
| Evolution of the energy spectra of anomalous cosmic rays in the outer heliosphere and the distance to the solar wind termination shock (p. 792) |
| by Stone, Edward C |
| EHE neutrinos from topological defects (p. 793) |
| by Yoshida, S |
| Positron propagation in MID-relativistic thermal plasmas (p. 794) |
| by Moskalenko, I V |
| The arrival directions of ultrahigh energy cosmic rays (p. 796) |
| by Afanasiev, B N |
| Radial and latitudinal gradients of anomalous cosmic rays in the outer heliosphere (p. 796) |
| by Stone, Edward C |
| Acoustic signals produced by ultrahigh energy neutrinos in water (p. 797) |
| by Dedenko, L G |
| Sensitivity of MACRO to U.H.E. neutrinos (p. 800) |
| by Corona, A |
| Radial and latitudinal gradients of anomalous cosmic ray oxygen throughout the heliosphere (p. 800) |
| by Cummings, A C |
| Study of the cosmic ray anisotropy at Eo - 100 TeV from EAS-TOP: 1992-1994 (p. 800) |
| by Aglietta, M |
| Mapping the earth's interior with astrophysical neutrinos (p. 804) |
| by Crawford, H J |
| Point source search for cosmic rays above 3X10 eV by AGASA (p. 804) |
| by Doi, T |
| Solar and interplanetary particles re-accelerated at the solar wind termination shock (p. 804) |
| by Mewaldt, R A |
| Point-source searches above 10 eV using the haverah Park Database (p. 808) |
| by Chikawa, M |
| Search for AGN v's with the Soudan 2 detector (p. 808) |
| by DeMuth, D M |
| Evidence for anomalous cosmic ray hydrogen during the 1976-1977 solar minimum (p. 808) |
| by Mewaldt, R A |
| The origin of the highest energy cosmic rays and the large scale structure of the universe (p. 809) |
| by Biermann, P L |
| Estimated flux limits for UHE neutrinos via acoustical detection techniques (p. 812) |
| by George, J |
| The deuterium/proton ratio as a measure of anomalous hydrogen (p. 812) |
| by Lopate, C |
| The design of a neutrino telescope using natural deep ice as a particle detector (p. 816) |
| by Gray, L |
| The reappearance of anomalous cosmic ray hydrogen (p. 816) |
| by Christian, E R |
| Point source search at great underground depth (p. 820) |
| by Adarkar, H |
| Energy spectrum of neutrino induced muons in deep underground calculated from the latest primary spectrum (p. 824) |
| by Bhattacharya, D P |
| Cosmic electron observations from the ice spacecraft (p. 824) |
| by Evenson, P |
| Calculation of muon flux at great depth produced neutrino from astronomical sources (p. 828) |
| by Battacharyya, D P |
| Solar modulation of hydrogen and helium cosmic ray nuclei spectra above 400 MeV/nucleon, from 1976 to 1993 (p. 828) |
| by Golden, R L |
| Recent production of the highest energy cosmic rays and the puzzles of their origin (p. 832) |
| by Bhattacharya, D P |
| Fluxes of ACR ions in the earth's magnetosphere at the end of the 22nd solar cycle (p. 832) |
| by Grigorov, N L |
| Investigation of GCR with the help of SONG instrument on-board KORONAS-I satellite (p. 836) |
| by Bogomolov, A V |
| Nestor, a neutrino astroparticle physic physics laboratory for the Mediterranean: The physics perspective (p. 836) |
| by Capone, A |
| Shadowing of cosmic rays by the sun near maximum or at the decreasing phase of solar activity (p. 840) |
| by Nishizawa, M |
| Search for magnetic monopoles with the Baikal neutrino telescope (p. 841) |
| by Belolaptikov, I A |
| Association of solar flare and radio burst with sunspot Magnetic field (p. 844) |
| by Gupta, D K |
| Search for dirac magnetic monopole production in high energy heavy ion collisions (p. 845) |
| by He, Y D |
| Peak flux density spectra of solar radio burst in relation to sunspot configuration (p. 848) |
| by Mishra, A P |
| Search for fast magnetic monopoles with the MACRO scintillator system (p. 849) |
| by Grassi, M |
| E - W distribution of solar LDE - Type flares and galactic cosmic Ray modulation ( 1969-1972) (p. 852) |
| by Jakimiec, M |
| Search for GUT monopoles with the MACRO streamer tube and track etch system (p. 853) |
| by Sciubba, A |
| Preliminary results of observations of relationships between solar radio bursts, sudden commencements on earth and interplanetary disturbances measured by (p. 856) |
| by Jansen, F |
| Cosmic ray signals from halo neutralinos (p. 857) |
| by Diehl, E |
| The features of the relationship of cosmic ray Forbush decreases and the solar wind parameters' fluctuations (p. 860) |
| by Alania, M V |
| Landau energy loss in liquid scintillator and the search for weakly interacting fractionally charged particles with the LVD experiment (p. 861) |
| by Fulgione, W |
| The development of observations and models of cosmic ray forbush-effects (p. 864) |
| by Dorman, I V |
| Particle dark matter search with low activity scintillators: An update (p. 865) |
| by Bacci, C |
| Regions of abnormally low proton temperature as signatures of ejecta in the solar wind and their solar cycle dependence (p. 868) |
| by Richardson, I G |
| Capture of galactic cold dark matter by the sun (p. 870) |
| by Mitra, A |
| Short-term cosmic ray decreases: 1964-1994 (p. 872) |
| by Cane, H V |
| Nal limits to cold galactic Dark matter interaction rates (p. 874) |
| by Quenby, J J |
| On structure of forbush effect on results of joint analysis od scintillation index and solar wind parameters (p. 876) |
| by Kozlov, V I |
| Possible candidates for cosmic ray anomalous massive particles (p. 878) |
| by Mori, K |
| Cosmic ray fluctuation power spectra dynamics during the great interplanetary disturbance on the October 19-21, 1989 (p. 880) |
| by Vashenyuk, E V |
| Search for neutron antineutron oscillations (p. 882) |
| by Adarkar, H |
| The angular extents of solar/interplanetary disturbances and modulation of galactic cosmic rays (p. 884) |
| by Cliver, E W |
| MINIMAX: a modest collider experiment to search for the centauro phenomenon: disoriented chiral condensates (p. 886) |
| by Jones, L W |
| Search for predictors of forbush decreases (p. 888) |
| by Belov, A V |
| Search for long-mean-free-path nuclei with a balloon-borne emulsion chamber (p. 890) |
| by Miyamura, O |
| The nature of cosmic ray forbush-decrease and precursory effects (p. 892) |
| by Dorman, L I |
| Search for isotropic gamma radiation between 65 and 200 TeV: constraints on topological defects and galactic dark matter in the form of molecular hydrogen (p. 894) |
| by Karle, A |
| Precursory decrease of cosmic rays, in front of forbush decrease associated IMF-shock wave, caused by CME lifting off the sun on april 14, 1994 (p. 896) |
| by Sakakibara, S |
| Anomalous massive particles in cosmic rays (p. 898) |
| by Saitô, T |
| Observation of GV protons associated with an interplanetary shock (p. 900) |
| by Humble, J E |
| High energy gravitons and prospects for detection (p. 902) |
| by Slobodrian, R J |
| The 24 March 1991 Forbush decrease (p. 904) |
| by Fluckiger, E O |
| Experiments of TL-stacks at the Mt. Blanc laboratory for heavy slowly particles (p. 906) |
| by Aglietta, M |
| An application of the pulse superposition method to cosmic ray time variations (p. 908) |
| by Petlenko, A V |
| Flux of hyper-strange matter on supersonic concord (p. 910) |
| by Capdevielle, J N |
| Anisotropy of cosmic rays and Forbush decreases in 1991 (p. 912) |
| by Belov, A V |
| The milagro data acquisition system (p. 914) |
| by Allen, G E |
| Characteristics of diurnal variations of cosmic rays and solar wind stream in Forbush decrease (p. 916) |
| by Darwish, A A |
| Water Cherenkov detectors for large air showers (p. 918) |
| by Yodh, G B |
| The dependence of solar diurnal variations of cosmic rays on Forbush decrease (p. 920) |
| by Darwish, A A |
| Glass RPCs for giant airshower detectors (p. 922) |
| by Nakamura, M |
| Effect of interplanetary magnetic clouds on cosmic ray diurnal anisotropy (p. 924) |
| by Chauhan, M L |
| Study of the punch-through of gamma showers in a muon detector and discrimination against hadron showers (p. 926) |
| by Ghesquière, C |
| Cosmic ray variations: Periodicities at T<24 hours (p. 928) |
| by Kudela, K |
| Mass resolution of ground based air shower experiments in the 10 to 10000 TeV range (p. 930) |
| by Yodh, G B |
| Study of cosmic ray daily variations during quiet periods at neutron monitor energies (p. 932) |
| by Agrawal, S P |
| Streamer tube muon detectors for kascade (p. 934) |
| by Doll, P |
| Long-term nature of the latitudinal cosmic ray gradient (p. 936) |
| by Darwish, A A |
| The new south pole air shower experiment spase 2 (p. 938) |
| by Beaman, J |
| High amplitude anisotropic wave train events in cosmic ray intensity during 1981-90 (p. 940) |
| by Kumar, S |
| The milagro detector (p. 942) |
| by Allen, G E |
| Anomalous behaviour of the low amplitude anisotropic wave trains in cosmic ray intensity during 1981-90 (p. 944) |
| by Kumar, S |
| Status and prospects of the EAS experiment KASCADE (p. 946) |
| by Klages, H O |
| Peculiar characteristics of low amplitude wave train events during solar cycle 21 (p. 948) |
| by Tiwari, A K |
| Design and performance of the lead-concrete Geiger tower array within the HEGRA experiment (p. 950) |
| by Rhode, W |
| Influence of coronal high-speed solar wind streams on cosmic ray intensity (p. 952) |
| by Sharma, N K |
| The AUGER project: first results from the Orsay prototype station (p. 954) |
| by Boratav, M |
| Ulysses observations of 26 day intensity variations of cosmic rays and anomalous helium over the south pole (p. 956) |
| by Zhang, M |
| A new system of high resolution imaging air Cherenkov telescopes for the Hegra experiment (p. 958) |
| by Panter, M |
| Corotating >60 MeV/amu cosmic ray depressions observed by spacecraft anti-coincidence guards (p. 960) |
| by Richardson, I G |
| On the optimal choice of EAS telescope-array in UHE ray astronomy (p. 962) |
| by Andreyev Yu M |
| Fractal analysis of cosmic ray signals detected in the EAS-TOP experiment (p. 964) |
| by Aglietta, M |
| Reflectometer for fast measurement of mirror reflectivity in the field (p. 966) |
| by Wild, N |
| Power spectrum of irregular time series of cosmic rays in a wide range of rigidity: 0.3-20 TeV (p. 968) |
| by Yasue, S I |
| Simulating high energy air showers at Soudan (p. 970) |
| by Border, P |
| The peculiarity of cosmic ray intensity of recurrent Forbush effects in two different 11-year cycles of solar activity (p. 972) |
| by Shatashvili, L Kh |
| Performance of cosmic rar tracking (CRT) detectors (p. 974) |
| by Bernlöhr, K |
| Cosmic ray modulation by expanding, high-latitudes streams (p. 976) |
| by Drolias, B |
| A new underground muon detector on MT Liang Wang (p. 978) |
| by Gao, X Y |
| On the potential of cosmic ray time variation studies with Milagro detector (p. 980) |
| by Ahluwalia, H S |
| Injection and fast radial diffusion of energetic electrons into the inner magnetosphere (p. 981) |
| by Gusev, A A |
| Coordinate detector for horizontal cosmic ray flux investigations (p. 982) |
| by Aglietta, M |
| Measurements of flux and spectrum of electrons with energy of 7 - 40 MeV near the earth (p. 985) |
| by Lupenko, G V |
| The effect of lead screen to scintillation detectors (p. 986) |
| by Luruoi, S |
| Nature of high energy electrons in the inner radiation belt (p. 989) |
| by Voronov, S A |
| âﾜGamma-raysâ bundies at the cores of extensive air showers and the primary cosmic ray identification (p. 990) |
| by Augusto, C R A |
| Electron and positron Albedo spectra with energy more than 20 MeV (p. 993) |
| by Koldashov, S V |
| Study of particle tracking from EASCAMP (p. 994) |
| by Biral, A R |
| Natural energetic positrons in the inner zone (p. 997) |
| by Martin, I M |
| A nucleonic inverse problem (p. 998) |
| by Portella, H M |
| An sonar triangulation system for position monitoring of the Baikal underwater array (p. 1001) |
| by Belolaptikov, I A |
| Chaos problem in the capture of anomalous cosmic ions (p. 1001) |
| by Pugacheva, G I |
| On the possible use of the solar power plant CESA-1 field at tabernas as Cerenkov detector (p. 1005) |
| by Plaga, R |
| Frift Hamiltonian in a dipole magnetic field (p. 1005) |
| by Nosov, S F |
| Remote surveys of AMANDA (p. 1009) |
| by Askebjer, P |
| Trapped oxygen and neon measurements on LDEF (p. 1009) |
| by Barz, S |
| Indirect Evidence for long absorption lengths in Antarctic ice (p. 1011) |
| by Tilav, S |
| Observations of geomagnetically trapped anomalous cosmic rays (p. 1013) |
| by Selesnick, R S |
| 1-20 KeV ion experiments with TL-Sheets (p. 1015) |
| by Kuga, K |
| Energy spectra of oxygen ions at E<40 MeV/nuc inside the magnetosphere (p. 1017) |
| by Leicher, M |
| SuperKamiokande outer DAQ system (p. 1019) |
| by Wilkes, R J |
| The isotopic composition of geomagnetically trapped helium (p. 1021) |
| by Wefel, J P |
| Radio detection of high energy showers (p. 1023) |
| by Alvarez-Muñiz, J |
| The energy spectra of interplanetary and trapped anomalous cosmic rays (p. 1025) |
| by Grigorov, N L |
| Using extra clear antartic ice as a supernova detector (p. 1027) |
| by Halzen, F |
| Differential flux measurement of atmospheric pion, muon electron and positron energy spectra at balloon altitudes (p. 1029) |
| by Grimani, C |
| Performance of transition radiation detector in MACRO (p. 1031) |
| by Spinelli, P |
| Atmospheric proton and deuterium energy spectra determination with the MASS2 (p. 1033) |
| by Papini, P |
| Ground level cosmic ray observations (p. 1037) |
| by Stephens, S A |
| Measurements of the absorption length of the ice at the South Pole in the Wavelength interval 410 nm to 610 nm (p. 1039) |
| by Erlandsson, B |
| He spectrum at small atmospheric depths for different geomagnetic cutoff values (p. 1041) |
| by Papini, P |
| Response of the NT-36 Array to a distant point-like light source (p. 1043) |
| by Belolaptikov, I A |
| Production of secondary deuterium in the atmosphere at various latitudes (p. 1044) |
| by Papini, P |
| A measurement of the fluorescence efficiency of air (p. 1047) |
| by Kakimoto, F |
| Secondary proton production at small atmospheric depths as a function of geomagnetic cut-off (p. 1047) |
| by Papini, P |
| Peculiarities of iron and subiron energy spectra at low energies (p. 1051) |
| by Baranov, D G |
| A project for a 17m imaging Cerenkov telescope (p. 1051) |
| by Bradbury, S M |
| Additional particle flux in upper earth atmosphere levels (p. 1055) |
| by Kolomeets, E V |
| Proposal to search for hypothetic heavy cosmic ray particles (p. 1056) |
| by Bazhutov, Yu N |
| The radial diffusion and the high frequency radio emission of energetic electrons of inner radiation belt during geomagnetic storm with D 110 nT (p. 1058) |
| by Dudnik A V |
| Data acquisition system for the Cherenkov water detector on the earth's surface (p. 1060) |
| by Aynutdinov, V M |
| The difference between offset dipole coordinates andcoordinates based on cutoff rigidity contours (p. 1062) |
| by Smart, D F |
| Study on the ELF?VLF noise for the nuclearites search experiment (p. 1064) |
| by Sasaki, H |
| Cosmic ray cutoff rigidities in the Tsyganenko magnetospheric magnetic field models of 1989 and 1987 years (p. 1066) |
| by Danilova, O A |
| Measurements with the altazimuthal counter telescope with a magnet spectrometer (p. 1068) |
| by Wada, T |
| Effects of the magnetosheath on cosmic ray particle propagation in near-earth space (p. 1070) |
| by Butikofer, R |
| Reconstruction of events in a water detector with quasispherical modules (p. 1072) |
| by Aynutdinov, V M |
| Cosmic ray asymptotic directions for Chilean neutron monitors (p. 1074) |
| by Storini, M |
| NEVOD - Neutrino water detector on the earth's surface (p. 1076) |
| by Aynutdinov, V M |
| Neutron monitor survey of the southern ocean (p. 1078) |
| by Bieber, J W |
| Present status of the NESTOR project (p. 1080) |
| by Bottai, S |
| Neutron monitor latitude surveys, response functions and 22-year modulation (p. 1082) |
| by Stoker, P H |
| A comparative study of geomagnetic storms for discrete activities during 1978-81 (p. 1086) |
| by Kumar, S |
| Magnetospheric effects of cosmic rays within the different phases of the magnetic storms (p. 1090) |
| by Baisultanova, L M |
| Fluctuations of cosmic rays of the geophysical origin (p. 1094) |
| by Antonova, V P |
| On a possibility of predicting the level of geomagnetic disturbance from effects in cosmic rays (p. 1098) |
| by Dvornikov, V M |
| The multiple relation among the cosmic ray geomagnetic activity and atmospheric noise (p. 1102) |
| by Szocs, H L |
| Forbush decreases as Indicators of health-hazardous geomagnetic storms (p. 1106) |
| by Villoresi, G |
| The influence of geomagnetic disturbances on the meteorological parameters in the BMA region (p. 1110) |
| by Pugacheva, G I |
| The precipitations of electrons into the earth's atmosphere during 1994 (p. 1114) |
| by Makhmutov, V S |
| Space shuttle measurements of the galactic cosmic radiation linear energy transfer spectra over a solar cycle and their comparison with radiation transport model (p. 1118) |
| by Badhwar, G D |
| Cosmic ray fluxes in atmosphere and precipitations (p. 1122) |
| by Stozhkov, Yu I |
| Solar protons from August 1972 flare and nitrate abundance in Antarctic snow (p. 1126) |
| by Gladysheva, O G |
| Unique possibility to obtain upper limit of total energy induced by solar flare protons (p. 1129) |
| by Gladysheva, O G |
| Polar cap intensity structures during the 22 july 1982 flare: correlation to interplanetary fluxes and anisitropies (p. 1133) |
| by Cooper, J F |
| GCR, the cirrus hole, global warming and record floods (p. 1137) |
| by Ely, J T |
| Temporal and latitudinal dependence of the temperature effect for neutron component if cosmic ray (p. 1141) |
| by Belov, A V |
| Modulation effect of barometric coefficient of neutron component of secondary cosmic rays (p. 1145) |
| by Yanchukovsky, V L |
| Day-night moon shadow difference and comparison with the sun shadow at 10 13 eV using the Tibet air shower array (p. 1148) |
| by Yamamoto, Y |
| The effect of neutron intensity increase formation during new-moon and full-moon period (p. 1151) |
| by Volodichev, N N |
| Energy deposit into the brain of an astronaut in space station by solar flare heavy particles (p. 1155) |
| by Young, P S |
| On a possible relationship between atmospheric dynamics ozone and global auroral activity (p. 1156) |
| by Marcucci, M F |
| On the theory of atmospheric electric field effect in cosmic ray muon component (p. 1160) |
| by Dorman, L I |
| On the possibility of atmospheric electric field effect in cosmic ray neutron component (p. 1164) |
| by Dorman, L I |
| Global ELF?VLF wave observation at the SL-9 comet crash on Jupiter (p. 1168) |
| by Chechin, V |
| Numerical simulations of Non-adiabatic particle motions in the jovian magnetosphere comparison with âﾜUlyssesâ observations (p. 1172) |
| by Drolias, B |
| The cyclic variations of the barometric coefficient of the cosmic ray neutron component intensity (p. 1176) |
| by Shatashvili, L |
| An influence of cosmic rays and geomagnetic disturbances on the cardiopathology tendency (p. 1180) |
| by Alania, M V |
| Solar flare tracks in Rio Negro (L4) chondrite (p. 1181) |
| by Bhandari, N |
| Cosmic ray gradients in the heliosphere based on isotope production rates in meteorites (p. 1184) |
| by Bhandari, N |
| Galactic cosmic ray variations over a scale of meteorite exposure ages (p. 1188) |
| by Alexeev, V A |
| GCR modulation in meteorites (p. 1192) |
| by Bonino, G |
| The solar signal in a 415-year nitrate record from a polar ice core (p. 1196) |
| by Dreschhoff, G A |
| Medium-and long-term cyclic variations of cosmic rays in the past (p. 1200) |
| by Dergachev, V A |
| Cosmogenic isotopes, geomagnetic and geochemical signals in a Mediterranean sea sediment at 35000 yr BP (p. 1204) |
| by Cini castagnoli, G |
| New model on solar neutrino (p. 1212) |
| by Yi-Fang, C |
| Are solar neutrinos electrically charged ? (p. 1216) |
| by Ignatiev, A Yu |
| Enhancement of the oscillations of neutrinos of different masses in matter (p. 1220) |
| by Beshtoev, K M |
| Implications of solar neutrino experiments for solar magnetic fields (p. 1228) |
| by Pandey, U C |
| Comments on a solar neutrino flux of the Kamiokande observation (p. 1231) |
| by Nakatsuka, T |
| Experimental limit on the solar antineutrino flux (p. 1235) |
| by Khalchukov, F F |
| The solar neutrino flux and heliolatitude anisotropy (p. 1239) |
| by Dorman, L I |
| Summary of correlative analyses between homestake neutrino data and parameters (p. 1243) |
| by Massetti, S |
| Green corona brightness and homestake neutrino data (p. 1247) |
| by Massetti, S |
| Is there a north-south asymmetry in the homestake neutrino data connected with solar activity ? (p. 1251) |
| by Massetti, S |
| Solar neutrino observations with superkamiokande (p. 1255) |
| by Conner, Z |
| Anticorrelation between neutrino flux and activity in the sun (p. 1259) |
| by Tomozawa, Y |
| Satellitte project PHOTON for study of the solar flare hard radiation (p. 1263) |
| by Kotov, Y D |
| Wide-band spectrometer of rays and neutrons for solar satellite project âﾜPHOTONâ (p. 1267) |
| by Kotov, Y D |
| Monte Carlo simulation of the response of inorganic scintillators to medium energy solar neutrons (p. 1271) |
| by Kotov, Y D |
| Anomalous and solar cosmic ray observations with the first brazilian scientific microsatellite (p. 1275) |
| by Turtelli, A |
| Performance of a magnet spectrometer based on digitzing optical spark chambers (p. 1279) |
| by Clem, J M |
| Silicon detector studies with an interferometric thickness mapper (p. 1283) |
| by Milliken, B |
| Specific energy loss rate measurements in low earth orbit (p. 1287) |
| by Williamson, P R |
| Large aperture muon hodoscope for studies in solar-terrestrial physics (p. 1291) |
| by Borog, V V |
| Internet access to NASA's OMNI and COHO data bases for interplanetary missions (p. 1295) |
| by Cooper, J F |
| Two-dimensional low power MWPC for long duration balloon flights (p. 1299) |
| by Moiseev, A A |
| The radiosonde for the neutron component of cosmic rays measurements in the strastosphere (p. 1304) |
| by Asatrian, G A |
| Solar physics with the Milagro telescope (p. 1308) |
| by Gisler, G |
| New experiment on the observation of solar neutrons at Chacataya (p. 1312) |
| by Matsubara, Y |
| Spaceship earth- An optimized Network of neutron monitors (p. 1316) |
| by Bieber, J W |
| Antarctic laboratory for cosmic rays: 1991-1995 (p. 1320) |
| by Cordaro, E G |
| The cosmic ray data database (p. 1324) |
| by Belov, A V |
| An application of cosmic rays for solving some ecology and hydrology problems (p. 1326) |
| by Fridman, Sh D |
| A real time compact monitor for environmental radiation: cosmic rays and radioactivity (p. 1329) |
| by Cecchini, S |
| Cosmic Ray propagation in turbulent media with non-zero helicity of random velocity field (p. 3001) |
| by Katz, M |
| Solar energetic electron events observed by phobos-2 (p. 3001) |
| by Stolpovski, V G |
| Is there a drift of anomalous cosmic ray particles? Measurements of the ULYSSES EPAC instrument (c820-823) |
| by Franz, M |
| The luminosity function of gamma-ray bursts (no pagination) |
| by Pizzichini, G |
| Atmospheric proton and deuterium energy spectra determination with the MASS2 experiment |
| by Papini, P |
| Measurement of the electron and positron energy differential fluxes with MASS2 apparatus |
| by Basini, G |
| Observations of cosmic ray positrons during the 1993 flight of the NMSU / WIZARD TS93 balloon borne apparatus |
| by Aversa, F |
| Cosmic ray anti-proton measurements in the 4-GeV - 19-GeV energy range using the NMSU / WIZARD matter antimatter superconducting spectrometer 2 (MASS2) |
| by Hof, M |
| anti-p and e+ identification capabilities of CAPRICE |
| by Barbiellini, G |
| Use of neural network techniques to identify cosmic ray electrons and positrons during the 1993 balloon flight of the NMSU/WIZARD TS93 instrument |
| by Bellotti, R |
| Cosmic ray spectrum and composition : direct observation |
| by Shibata, T |
| Violation of Feynman scaling law in the forward region |
| by Ohsawa, A |