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Pinoybix Radiowave Key

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1.

field strength

2. both electric and magnetic fields.

3. D

4. James Clerk Maxwell

5. Kennely – Heaviside Layers

6. band

7. 90 degrees

8. a magnetic field

9. space waves

10. is due to the transverse nature of the waves

11. pass into a medium of different dielectric constants

12. ionosphere

13. F2

14. K factor

15. reflection-multipath

16. D Layer

17. E Layer

18. critical frequency

19. 3 to 30MHz

20. 0.3 to 3MHz

21. scatter angle

22. lengthen the skip distance

23. volts per meter


24. all of the above

25. polarization

26. circularly polarized

27. 300×106 m/s

28. 317 W

29. Plane wave

30. is less than that in A

31. is a universal constant

32. always seems less than its actual depth

33. a fixed point in an electromagnetic wave

34. 1 W

35. electric field

36. shading of the RF signal by hills and trees

37. vertical

38. horizontal

39. vertical

40. an electric field and a magnetic field

41. it is more pronounced at wide bandwidths

42. spread spectrum communication

43. electric field

44. knife-edge diffraction

45. is greater than 1

46. approximately 300 million m/s


47. 8500 km

48. 1.23

49. vertical polarization

50. horizontal polarization


51. fading

52. they are very reliable

53. 12 GHz

54. affected by the solar cycle

55. to prevent sky-wave and upper ray interference

56. frequency diversity

57. window

58. space waves

59. UHF

60. tilting

61. the physical orientation of electric field in space

62. attenuation

63. their frequency

64. may occur around the edge of a sharp object

65. Perpendicular to both the magnetic field and the wave direction

66. X-rays

67. Energy

68. Long distance radio communication

69. Blue

70. Pitch
71. Can appear on screen

72. Frequency

73. Either A or B above

74. Dependent on the indexes of refraction of the two media

75. E layer

76. The splitting of white light into its component colors in refraction

77. Always seems less than its actual depth

78. That has a lower index of refraction

79. 90 degrees

80. Candela

81. Low-wattage light bulb

82. 8000 lx

83. 18 degrees

84. 0 degrees

85. 1.52

86. 1.3

87. 60 degrees

88. 2 π sr

89. 1508 lx

90. Direct wave

91. Refracted

92. 300 KHz to 3 MHz

93. 3 to 30 MHz
94. Sky wave

95. HF

96. 53.2 mi

97. Increase antenna height

98. Inverse square law

99. Sky wave

100. F2
101. E

102. Ultraviolet radiation

103. F2

104. All of these

105. All of these

106. MUF

107. Skip distance

108. Fading

109. Space diversity

110. Frequency diversity

111. Diversity

112. Solar flares

113. SIDs

114. Troposcatter propagation

115. Troposcatter

116. Ducting
117. Duct

118. Electric field

119. Shadow zone

120. Huygen’s principle

121. Troposphere

122. At midday

123. Afternoon or early evening

124. Very high and ultra high frequencies

125. F2 layer

126. window

127. scatter angle

128. diplexer

129. faraday effect

130. angle diversity

131. hectometric wave

132. F2

133. LF

134. 3 – 30 GHz

135. vertical polarization

136. is horizontal

137. 3

138. ground

139. increases
140. long

141. makes more dense and irregular

142. ionosphere, ground, ionosphere and back to ground

143. ionosphere variation

144. between end of ground and first reflected wave

145. ground

146. to take advantage of best reflected signals

147. VHF and UHF

148. water

149. static

150. vertical
201. Ground wave

202. VLF and LF

203. time diversity

204. Any of these

205. window

206. Polarization

207. 7.96 µW/m^2

208. tilting

209. Horizontal

210. 21 km

211. MF, HF

212. ducting

213. Circularly polarized


214. Direct waves

215. seasonal variation

216. 23.9 GW/m^2

217. point source

218. may occur around the edge of a sharp obstacle

219. 34 MHz

220. power density

221. 10.3 degrees

222. field intensity

223. James Clerk Maxwell

224. UHF

225. any of these

226. height

227. 1.15

228. refraction

229. attenuation

230. multi-hop transmission

231. pass into a medium of different dielectric constant

232. absorption

233. sky wave signal

234. Selective fading

235. diffraction

236. Amplitude modulation


237. Huygen’s principle

238. 8.66 mW/m

239. their frequency

240. 37.9 mi

241. 2.03 x 10^-12 W

242. attenuation

243. Terrestrial wave

244. 6.35 x 10^ -16 W/m^2

245. fading

246. isothermal region

247. sunspot

248. is due to the transverse nature of the waves

249. Surface waves

250. Space waves


251. Radio horizon

252. sky waves

253. skipping

254. Electromagnetic waves

255. D layer

256. ghosting

257. MF and HF

258. Kennely-Heavisides

259. critical frequency


260. critical angle

261. wavefront

262. virtual height

263. maximum usable frequency

264. E field

265. optimum working frequency

266. skip distance

267. Pedersen ray

268. EMI

269. quiet zone

270. RFI

271. any of these

272. increase antenna height

273. 142 dB

274. 53.2 mi

275. Fading

276. HF

277. they are very reliable

278. direct wave

279. 12 GHz

280. sky wave

281. affected by the solar cycle

282. 3 to 30 MHz
283. to prevent sky-wave and upper ray interference

284. 300 kHz to 3 MHz

285. refracted

286. the Faraday effect

287. frequency diversity

288. reflection coefficient

289. solar flux

290. Maunder period

291. tilting

292. Troposphere

293. LUF

294. skip zone

295. diurnal variation

296. Any of these

297. polarization fading

298. one-third

299. temperature inversion

300. duct
301. The direction in which the electric plane is radiated.

302. Kenelly Heaviside Layers

303. Wave impedance

304. The field strength

305. Law of Reciprocity

306. VHF and above


307. Ground wave

308. space waves

309. diffraction

310. attenuation

311. Vertically and horizontally polarized separately

312. Horizontally

313. Permitivity

314. Huygen’s Principle

315. Velocity factor

316. Diffraction

317. Line of sight propagation wave

318. Radiation pattern

319. Permittivity

320. Surface wave propagation

321. Either a or b

322. Virtual height

323. Critical frequency

324. Both a and b

325. The magnitude of the incident is equal to the reflected waves

326. Refraction

327. Snell’s Law

328. D layer

329. Thermal inversion


330. E-layer

331. All of these

332. F layer

333. Space or direct

334. Inverse Square Law

335. 2

336. Sporadic E

337. Attenuation

338. Wave propagation

339. Carrier frequency

340. Transverse waves

341. Fading

342. They are very reliable

343. Affected by the solar cycle

344. To prevent sky-wave and upper ray interference

345. Tilting

346. Is due to the transverse nature of the waves

347. Log normal fading

348. Their frequency

349. Pass into a medium of different dielectric constant

350. Arises only with spherical wavefronts


351. All of these

352. Oscillations that propagate through free space


353. Electric field

354. Electric field (E-field) and magnetic field

355. Wavefront

356. Ray

357. Power density

358. Field intensity

359. A or C is correct

360. Inductance

361. B or C is correct

362. A and B

363. A or C is right

364. Smaller value of dielectric constant

365. The ratio of velocity of light in free space to the velocity of light in a given material

366. A and B are incorporated

367. A and B

368. Is a reflection from a perfectly smooth surface

369. Rayleigh criterion

370. Standing waves

371. Interference

372. Isotropic source

373. 300,000 km/sec

374. Magnetic field

375. Measures power density, magnetic field intensity, and electric field intensity
376. Should take place at one medium

377. All of these

378. Ground wave

379. Gradient density

380. B and C

381. All of these

382. Radio horizon

383. All of the above

384. All of these

385. Duct propagation

386. Increase

387. Increasing refraction

388. B or C

389. A and C

390. E layer

391. F layer

392. Virtual height

393. Skip distance

394. Maximum usable frequency, MUF

395. Multihop transmission

396. Hop

397. Fading

398. Diversity techniques

399. Frequency diversity


400. Space diversity

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