Astrophysics (Index)About

electromagnetic radiation

(EMR, EM radiation, radiation, electromagnetic waves)
(radiation such as light, radio, X-rays)

Electromagnetic radiation (EM radiation or EMR or just radiation) is radiation such as light, radio waves, etc. (Much of the dangerous radiation associated with radioactivity is not EMR: much EMR is ubiquitous and harmless in everyday life.) EMR is termed "electromagnetic" because modeling of the nature of electric fields and magnetic fields showed that changes in either produce the other, which can happen such that changes back and forth can propagate as waves, and such waves were deliberately produced by manipulating electric and magnetic fields, producing what we call radio waves. Both in theory and in experiment, these waves showed properties like those of light (such as the same speed, i.e., c), exactly as if light and radio waves are the same thing, except for their frequency. Overall classifications within the electromagnetic spectrum (based on wavelength/frequency ranges):

For more detail, see electromagnetic spectrum and the Wavelengths Table.


(physics,electromagnetism)
Further reading:
https://en.wikipedia.org/wiki/Electromagnetic_radiation
https://en.wiktionary.org/wiki/electromagnetic_radiation
https://astronomy.swin.edu.au/cosmos/E/Electromagnetic+Radiation
http://hyperphysics.phy-astr.gsu.edu/hbase/Waves/emwv.html
https://www.expii.com/t/electromagnetic-radiation-overview-types-8301
https://www.physics.umd.edu/courses/Phys122/Streets/25_EM_Induction_and_Waves.pdf
https://chem.libretexts.org/Bookshelves/Physical_and_Theoretical_Chemistry_Textbook_Maps/Supplemental_Modules_(Physical_and_Theoretical_Chemistry)/Spectroscopy/Fundamentals_of_Spectroscopy/Electromagnetic_Radiation

Referenced by pages:
1.3-mm observation
21-cm line
AB system
absorption
absorption coefficient
absorption line
accretion disk
active galactic nucleus (AGN)
advection dominated accretion flow (ADAF)
Airy disk
albedo
ALMACAL
amplitude
angstrom (Å)
angular power spectrum
antenna pattern
antenna temperature
apodization
ARCADE
astronomical quantities
astronomical survey
atmosphere
atmosphere formation
atmospheric escape
atmospheric window
atomic dark matter (aDM)
aurora
Balmer series (H)
Balmer-break galaxy (BBG)
band shifting
bandpass filter
baryon acoustic oscillations (BAO)
beam
beat frequency
Big Bang
biosignature
black body (BB)
black hole (BH)
black hole binary (BHB)
black hole shadow
black-body radiation
blazar
blue shift
bolometer
bolometric correction
bolometric luminosity (LBol)
bolometric magnitude (Mbol)
BOOMERanG
Brackett series
bremsstrahlung
brightness temperature (TB)
carbon (C)
carbon dioxide (CO2)
Castro
cavity-enhanced absorption spectroscopy (CEAS)
CCD
Cherenkov radiation
chopping mirror
chromatic aberration
circular polarization ratio (CPR)
circumstellar disk
Cloudy
CMB polarization
coherent light
cold gas
cold mass accretion (CMA)
collecting area
color temperature (TC)
COMAP
Compton reflection
Compton scattering
Compton telescope
continuous absorption
continuum emission
corona
cosmic background radiation (CBR)
cosmic dust
cosmic gamma ray background (CGB)
cosmic infrared background (CIB)
cosmic microwave background (CMB)
cosmic optical background (COB)
cosmic rays (CR)
cosmic X-ray background (CXB)
cosmology
counterpart
critical density (ρc)
current sheet
curvature radiation
cyclotron radiation
damped Lyman alpha absorber (DLA)
dark galaxy
dark matter (DM)
dark matter detector
dark matter filament
dark nebula
deep survey
density parameter
differential spectroscopy
diffuse emission
dispersion measure (DM)
Doppler shift
Dragone telescope
dropout
dust echo
dusty galaxy
earthshine
eccentricity (e)
Eddington approximation
effective temperature (Teff)
Einstein coefficients
Einstein delay
electric dipole radiation
electromagnetic spectrum
electromagnetism (EM)
electron orbital
electron scattering
electron volt (eV)
emission
emission coefficient (j)
emission line
emission nebula
emission-line star
emissivity
energy
energy density
epoch of reionization (EOR)
equation of radiative transfer (RTE)
equilibrium temperature (Teq)
escape fraction
escape velocity (Ve)
etalon
event horizon (EH)
extragalactic background light (EBL)
extreme ultraviolet (EUV)
extremely low frequency (ELF)
Fanaroff-Riley classification
far infrared (FIR)
Faraday rotation
filter
fluorescence
flux
flux density
flux reconstruction (FR)
foreground subtraction
Fourier series
Fourier transform (FT)
frame of reference
frequency (ν)
fusion
galactic disk
galactic electron density
galaxy formation
gamma rays (GR)
gamma-ray burst (GRB)
geodesic
Geroch-Bekenstein engine
grating
gravimetry
gravitational lensing
gravitational potential energy
gravitational redshift
gravitational wave (GW)
gravitational wave spectrum
gravitational-wave detector
graviton
gravity
gray body
grazing incidence optics (GIO)
greenhouse effect
grism
Gunn-Peterson trough
GW170817
habitability
Hanbury Brown and Twiss effect (HBT effect)
Hanle effect
HARM²
Hawking radiation
helium rain
heterodyne spectrometer
high-energy astrophysics (HEA)
HII region (HII)
HITEMP
HITRAN
hot DOG
Humphreys series
hydrodynamic escape
hydrodynamics
hydrogen (H)
hypermassive neutron star (HMNS)
IMB
in situ
inflated radii
infrared (IR)
infrared excess (IRX)
insolation
intensity
interference
interferometry
intergalactic medium (IGM)
interstellar holography
interstellar radiation field (ISRF)
inverse square law
ionized hydrogen (HII)
ionizing radiation
ionosphere
irradiance
isophote
isotropy
Kelvin-Helmholtz mechanism (KH mechanism)
KID
kilonova (KN)
Kirchhoff's law of thermal radiation
Klein-Nishina formula
Kramers opacity law
Lambda-CDM model (ΛCDM)
light cone
light curve
light echo
limb
line blanketing
line broadening
local thermodynamic equilibrium (LTE)
luminosity distance (dL)
luminous infrared galaxy (LIRG)
Lyman alpha (Ly-α)
Lyman beta (Ly-β)
Lyman series (L)
Lyman-alpha blob
Lyman-alpha forest
Lyman-break galaxy (LBG)
Lyman-Werner photon
M-type star (M)
MACHO
magnetic dipole radiation
magnitude
maser
Maxwell's equations
microcalorimeter
microchannel array
microwave
Mie scattering
millimeter astronomy
MITgcm
molecular cloud
molecular handedness
multi-messenger astronomy (MMA)
natural astronomical telescopes
neutrino observatory
neutron scattering
neutron star (NS)
NGC 3314
nitrogen (N)
noise-equivalent power (NEP)
non-thermal emission
observable universe
observational astronomy
occultation
OH/IR source
one dimensional climate model
optical depth (τ)
optics
orbital decay
PAH emissions
panchromatic
partial ionization zone
parts per million (PPM)
Paschen series
Pfund series
photocathode
photodiode
photodissociation region (PDR)
photoevaporation
photometric system
photometry
photomultiplier tube (PMT)
photon
photon counting
photon energy
photon noise
photosphere
Planck function
planet structure
point source
point-spread function (PSF)
polarimetry
polarization
Population I (Pop I)
Population II (Pop II)
power law
Poynting vector (S)
proportional counter
protogalaxy
protoplanetary disk (PPD)
proximity effect
pulsar (PSR)
pulsar timing array (PTA)
quantum
quantum efficiency (QE)
quark
quasi-periodic oscillation (QPO)
radiance
radiation belt
radiation era
radiation hydrodynamics (RHD)
radiation pressure
radiation zone
radiative flux
radiative forcing (RF)
radiative transfer (RT)
radiative transfer code (RT code)
radio
radio galaxy (RG)
radio relics
radio telescope
radioactivity
radiolysis
radiometer
Rayleigh scattering
Rayleigh-Jeans law
red giant
redshift (z)
reflection nebula
reflector telescope
refraction
refractive index
relativistic beaming
relativity
rest wavelength
RMS astronomy
rocky planet
Roemer delay
Rosseland mean opacity
Sachs-Wolfe effect (SWE)
scattering
Schuster-Schwarzschild model
self-absorption
sensitivity function (S)
Shapiro delay
shock wave
SIMSTACK
sky subtraction
SMBH formation
SN 1987A (1987A)
Solar and Heliospheric Observatory (SOHO)
solar constant
solid angle (Ω)
source
source function (S)
specific intensity
speckles
spectral density
spectral energy distribution (SED)
spectral flux density (S)
spectral index (α)
spectral line
spectral line shape
spectral power distribution (SPD)
spectral signature
spectral temperature
spectrometer
spectropolarimetry
spectroscopy
SPECULOOS
speed of light (c)
spin-down luminosity
standard model of a flare
standard siren
star
star formation (SF)
star formation feedback
star formation history (SFH)
starburst galaxy
stellar atmosphere
stellar flare
stellar model atmosphere
stellar population
stellar structure
stellar temperature determination
stimulated emission
Stokes parameters
stray light
submillimeter astronomy
submillimeter galaxy (SMG)
subradio
sunspot
super low frequency (SLF)
superconducting tunnel junction (STJ)
superluminal motion
superluminous supernova (SLSN)
supernova designator
supernova light curve (SN light curve)
supernova remnant (SNR)
superradiance
surface temperature
synchrotron radiation
synchrotron self-Compton (SSC)
systematic error
tau neutrino (ντ)
technosignature
telescope
telescope type
temperature
thermal bremsstrahlung
thermal emission
thermal inertia
thin disk
Thomson optical depth (τT)
Thomson scattering
three dimensional model
tidal disruption event (TDE)
time-delay cosmology
TIMED
timescale (t)
tired light
Titan
tomography
transient (AT)
transit spectroscopy
transiting planet
transition edge sensor (TES)
transmission spectroscopy
tremendously low frequency (TLF)
two-stream approximation
Type Ia supernova
ultra low frequency (ULF)
ultraviolet (UV)
vegetation red edge (VRE)
velocity dispersion (σ)
very low frequency (VLF)
visible light
water lines
watt (W)
wave-particle duality
wavefront error (WFE)
wavefront sensor (WFS)
wavelength (λ)
wavenumber (ν)
waveplate
weak lensing (WL)
white dwarf (WD)
Wien approximation
Wien's displacement law
WIMP
Wolter telescope
X-ray
X-ray pulsar
XEUV
Yarkovsky effect
Yarkovsky-O'Keefe-Radzievskii-Paddack effect (YORP)
Zanstra method
ZEPLIN
zone of avoidance (ZOA)

Index