Astrophysics (Index)About

frequency

(number of cycles per unit of time, such as waves per second)

Frequency is the number of cycles per unit time. Typical measurement is in hertz, number of cycles per second. In astrophysics, the term frequency is often used for electromagnetic radiation (EMR), the rate at which individual waves are sent or received. For EMR, the wavelength times the frequency is equal to the speed of light. The energy of a photon is directly related to its EMR frequency:

E = h × f

Frequency, wavelength, and photon energy offer three means of quantifying the same characteristic of EMR: frequency is often cited for the longest wavelengths (radio and microwave), and photon energy for the shortest (X-rays and gamma rays), with wavelength commonly used for visible light and the surrounding regions of the spectrum.

The term frequency is also used for other cycling astronomical phenomena such as regularly pulsing radiation (e.g., from pulsars).


(EMR,measure,waves)
Further reading:
http://en.wikipedia.org/wiki/Frequency

Referenced by pages:
absorption line
AB system
ACIS
Atacama Cosmology Telescope (ACT)
anomalous microwave emission (AME)
anisotropy
antenna temperature
Archeops
Allen Telescope Array (ATA)
Australia Telescope Compact Array (ATCA)
bandwidth
black hole merger
black-body radiation
Bohr model
bolometer
Cambridge Catalog of Radio Sources (C)
C-BASS
Canadian Hydrogen Intensity Mapping Experiment (CHIME)
chirp
chirp mass (Mc)
cosmic microwave background (CMB)
carbon monoxide (CO)
Compton reflection
Compton scattering
CONCERTO
Cosmic Explorer
corotation resonance (CR)
cyclotron radiation
data cube
de Broglie wavelength
degeneracy
velocity dispersion (σ)
dispersion measure (DM)
Doppler broadening
Doppler shift
downconverter
Earth-sized VLBI
Effelsberg 100-m Radio Telescope
eigenmode
Einstein Telescope
electromagnetic spectrum
electron orbital
electron shell
extremely low frequency (ELF)
electromagnetic radiation (EMR)
epicyclic frequency
electron volt (eV)
fluorescence
flux density
frequency modulation (FM)
Fourier space
Fourier transform
fast radio burst (FRB)
galactic electron density
galaxy power spectrum
gamma rays (GR)
Green Bank Telescope (GBT)
gravitational wave (GW)
gravitational-wave detector
gravitational wave spectrum
gravitational wave strain (h)
habitable zone (HZ)
Hadley cell
hardness
Hellings and Downs curve
high frequency (HF)
infrared (IR)
interference
ionosphere
International Pulsar Timing Array (IPTA)
irradiance
Infrared Survey Facility (IRSF)
jansky (Jy)
Klein-Nishina formula
low frequency radio astronomy
LIGO
Lunar Reconnaissance Orbiter (LRO)
Crab Nebula (M1)
maser
microwave
multichroic feedhorn array
multi-messenger astronomy
Next Generation Very Large Array (ngVLA)
nanohertz gravitational waves
Nançay Radio Telescope (NRT)
neutron star merger
opacity (κ)
optical depth (τ)
passband
phased array
photoionization
photon
Parkes Catalog (PKS)
Planck
Planck constant (h)
plasma frequency
power law
pulsar timing array (PTA)
precipitable water vapor (PWV)
quad-ridge flare horn (QRFH)
quantum
radiance
radiant flux
radio
radio astronomy
radiometer equation
Rayleigh-Jeans law
red noise
radio frequency interference (RFI)
RMS astronomy
Rossby number (Ro)
Rosseland mean opacity
equation of radiative transfer (RTE)
scintillometry
spectral energy distribution (SED)
sensitivity function (S)
Square Kilometre Array (SKA)
super low frequency (SLF)
Solar and Heliospheric Observatory (SOHO)
spectral power distribution (SPD)
specific intensity
spectral correlator
spectral density
spectral flux density (S)
spectral index (α)
spectral line designation
spectral method
SPIDER
spinning dust emission
spiral galaxy
South Pole Telescope (SPT)
Sardinia Radio Telescope (SRT)
synchrotron self-Compton (SSC)
standard model of a flare
superconducting tunnel junction (STJ)
subradio
sunspot
superradiance
synchrotron radiation
Sunyaev-Zel'dovich effect (SZ effect)
telegrapher's equations
Thermal Bremsstrahlung
Thomson scattering
time series analysis
tremendously low frequency (TLF)
ultra low frequency (ULF)
Virgo
very low frequency (VLF)
Very Small Array (VSA)
wavelength
wavenumber
wave-particle duality
wavefront error (WFE)
Wien approximation
Wien's displacement law
atmospheric window
X-ray

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