- Cosmic noise
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Cosmic noise and galactic radio noise is random noise that originates outside the Earth's atmosphere. It can be detected and heard on radio receivers.
Elaboration
Cosmic noise characteristics are similar to those of thermal noise. Cosmic noise is experienced at frequencies above about 15 MHz when highly directional antennas are pointed toward the sun or to certain other regions of the sky such as the center of the Milky Way Galaxy. Celestial objects like Quasars, super dense objects that lie far from Earth, emit electromagnetic waves in its full spectrum including radio waves. We can also hear the fall of a meteorite in a radio receiver; as the falling object burns from friction with the Earth's atmosphere, ionizing surrounding gases, thereby producing radio waves. Cosmic Microwave Background Radiation (CMBR) from outer space, discovered by Arno Penzias and Robert Wilson, who later won the Nobel Prize for this discovery, is also a form of cosmic noise. CMBR is thought to be a relic of the Big Bang, and pervades the space almost homogeneously over the entire celestial sphere. The bandwidth of the CMBR is wide, though the peak is in the microwave range.
See also
- Intergalactic space
- Interplanetary space
- Interstellar medium
- Radio astronomy
References
This article incorporates public domain material from the General Services Administration document "Federal Standard 1037C" (in support of MIL-STD-188).
Noise (in physics and telecommunications) General Noise in... Class of noise Additive white Gaussian noise (AWGN) · Atmospheric noise · Background noise · Brownian noise · Burst noise · Cosmic noise · Flicker noise · Gaussian noise · Grey noise · Jitter · Johnson–Nyquist noise · Pink noise · Quantization error (or q. noise) · Shot noise · White noiseEngineering terms Ratios Carrier-to-noise ratio (C/N) · Carrier-to-receiver noise density (C/kT) · dBrnC · Eb/N0 (energy per bit to noise density) · Es/N0 (energy per symbol to noise density) · Modulation error ratio (MER) · Signal, noise and distortion (SINAD) · Signal-to-interference ratio (S/I) · Signal-to-noise ratio (S/N, SNR) · Signal to noise ratio (imaging) · Signal-to-noise plus interference (SNIR) · Signal-to-quantization-noise ratio (SQNR)Related topics Categories:- Astronomical radio sources
- Noise
- Astronomy stubs
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