Radio Wave Radio Waves Are A Type of Electromagnetic Radiation With Wavelengths in
Radio Wave Radio Waves Are A Type of Electromagnetic Radiation With Wavelengths in
Radio Wave Radio Waves Are A Type of Electromagnetic Radiation With Wavelengths in
Microwaves travel by line-of-sight; unlike lower frequency radio waves they do not
diffract around hills, follow the earth's surface as ground waves, or reflect from the ionosphere, so
terrestrial microwave communication links are limited by the visual horizon to about 40 miles (64
km). At the high end of the band they are absorbed by gases in the atmosphere, limiting practical
communication distances to around a kilometer. Microwaves are widely used in modern technology,
for example in point-to-point communication links, wireless networks, microwave radio relay
networks, radar, satellite and spacecraft communication, medical diathermy and cancer treatment,
remote sensing, radio astronomy, particle accelerators, spectroscopy, industrial heating, collision
avoidance systems, garage door openers and keyless entry systems, and for cooking food in
microwave ovens.
INFRARED WAVE
Infrared radiation was discovered in 1800 by astronomer Sir William Herschel, who
discovered a type of invisible radiation in the spectrum lower in energy than red light, by means of
its effect on a thermometer.[6] Slightly more than half of the total energy from the Sun was
eventually found to arrive on Earth in the form of infrared. The balance between absorbed and
emitted infrared radiation has a critical effect on Earth's climate.
Extensive uses for military and civilian applications include target acquisition,
surveillance, night vision, homing, and tracking. Humans at normal body temperature radiate chiefly
at wavelengths around 10 μm (micrometers). Non-military uses include thermal efficiency analysis,
environmental monitoring, industrial facility inspections, detection of grow-ops, remote
temperature sensing, short-range wireless communication, spectroscopy, and weather forecasting.
The visible spectrum is the portion of the electromagnetic spectrum that is visible to the
human eye. Electromagnetic radiation in this range of wavelengths is called visible light or simply
light. A typical human eye will respond to wavelengths from about 380 to 740 nanometers.[1] In
terms of frequency, this corresponds to a band in the vicinity of 430–770 THz.
The spectrum does not contain all the colors that the human eyes and brain can distinguish.
Unsaturated colors such as pink, or purple variations like magenta, for example, are absent because
they can only be made from a mix of multiple wavelengths. Colors containing only one wavelength
are also called pure colors or spectral colors.
Visible wavelengths pass largely unattenuated through the Earth's atmosphere via the
"optical window" region of the electromagnetic spectrum. An example of this phenomenon is when
clean air scatters blue light more than red light, and so the midday sky appears blue (apart from the
area around the sun which appears white because the light is not scattered as much). The optical
window is also referred to as the "visible window" because it overlaps the human visible response
spectrum. The near infrared (NIR) window lies just out of the human vision, as well as the medium
wavelength infrared (MWIR) window, and the long wavelength or far infrared (LWIR or FIR) window,
although other animals may experience them.
ULTRAVIOLET WAVE
Ultraviolet (UV) is electromagnetic radiation with wavelength from 10 nm to 400 nm, shorter
than that of visible light but longer than X-rays. UV radiation is present in sunlight, and constitutes
about 10% of the total electromagnetic radiation output from the Sun. It is also produced by electric
arcs and specialized lights, such as mercury-vapor lamps, tanning lamps, and black lights. Although
long-wavelength ultraviolet is not considered an ionizing radiation because its photons lack the
energy to ionize atoms, it can cause chemical reactions and causes many substances to glow or
fluoresce. Consequently, the chemical and biological effects of UV are greater than simple heating
effects, and many practical applications of UV radiation derive from its interactions with organic
molecules.
Short-wave ultraviolet light damages DNA and sterilizes surfaces with which it comes into
contact. For humans, suntan and sunburn are familiar effects of exposure of the skin to UV light,
along with an increased risks of skin cancer. The amount of UV light produced by the Sun means that
the Earth would not be able to sustain life on dry land if most of that light were not filtered out by
the atmosphere.[1] More energetic, shorter-wavelength "extreme" UV below 121 nm ionizes air so
strongly that it is absorbed before it reaches the ground.[2] However, ultraviolet light is also
responsible for the formation of bone-strengthening vitamin D in most land vertebrates, including
humans (specifically, UVB).[3] The UV spectrum thus has effects both beneficial and harmful to life.
The lower wavelength limit of human vision is conventionally taken as 400 nm, so ultraviolet
rays are invisible to humans, although some people can perceive light at slightly shorter wavelengths
than this. Insects, birds, and some mammals can see near-UV (i.e. slightly shorter wavelengths than
humans can see).
X-RAY
Gamma rays from radioactive decay are in the energy range from a few kiloelectronvolts
(keV) to approximately 8 megaelectronvolts (~8 MeV), corresponding to the typical energy levels in
nuclei with reasonably long lifetimes. The energy spectrum of gamma rays can be used to identify
the decaying radionuclides using gamma spectroscopy. Very-high-energy gamma rays in the 100–
1000 teraelectronvolt (TeV) range have been observed from sources such as the Cygnus X-3
microquasar.
Natural sources of gamma rays originating on Earth are mostly as a result of radioactive
decay and secondary radiation from atmospheric interactions with cosmic ray particles. However,
there are other rare natural sources, such as terrestrial gamma-ray flashes, which produce gamma
rays from electron action upon the nucleus. Notable artificial sources of gamma rays include fission,
such as that which occurs in nuclear reactors, and high energy physics experiments, such as neutral
pion decay and nuclear fusion.
Gamma rays and X-rays are both electromagnetic radiation, and since they overlap in the
electromagnetic spectrum, the terminology varies between scientific disciplines. In some fields of
physics, they are distinguished by their origin: Gamma rays are created by nuclear decay, while in
the case of X-rays, the origin is outside the nucleus. In astrophysics, gamma rays are conventionally
defined as having photon energies above 100 keV and are the subject of gamma ray astronomy,
while radiation below 100 keV is classified as X-rays and is the subject of X-ray astronomy. This
convention stems from the early man-made X-rays, which had energies only up to 100 keV, whereas
many gamma rays could go to higher energies. A large fraction of astronomical gamma rays are
screened by Earth's atmosphere.
Gamma rays are ionizing radiation and are thus biologically hazardous. Due to their high
penetration power, they can damage bone marrow and internal organs. Unlike alpha and beta rays,
they pass easily through the body and thus pose a formidable radiation protection challenge,
requiring shielding made from dense materials such as lead or concrete.