Astrophysics (Index)About

emission

(addition of photons to a beam of EMR)

The term emission has a particular meaning in the study of radiative transfer and spectroscopy, meaning the addition of photons to a beam of electromagnetic radiation (e.g., light), such as from changes in atoms, and also from scattering. It is the inverse of absorption, the removal of photons to the beam. The concept is used widely in astrophysics, for explaining and modeling stars, for dealing with the effects of the Earth's atmosphere, for explaining and modeling gas clouds, etc. Each type of emission has an absorption analog (though scattering is both emission and absorption), thus the classification of emission processes also is a classification of absorption processes.

Spontaneous emission is the emission of a photon by an atom not from any immediate interaction, such as the emission of a photon when an atom a lower level of atomic excitation (when an electron moves to a lower orbit). The both the time direction of the emitted photon are random.

Stimulated emission is the emission of a photon by a similarly-excited atom but the emission is specifically triggered by a passing photon of a wavelength that the atom is prepared to emit (i.e., it is excited such that it could emit a photon of this wavelength by spontaneous emission). In this case, the emitted photon has the same characteristics as the photon that stimulated the emission, including its direction. Such stimulated emission is also referred to as negative absorption: on a macro scale, absorption suggests EMR passing through some material is attenuated, but if stimulated emission is occurring, it is possible that more EMR at the wavelength exits than entered. Masers and lasers are based on this effect, by setting up a configuration so that the "doubling" of photons happens repeatedly.

Emission through scattering includes photons entering the beam through Thomson scattering or Compton scattering.


The term emission is also used within astronomy in a more general sense, for the EMR produced by some object, and also for other produced particles (e.g., neutrinos) or waves (gravitational waves).


(physics,EMR,radiative transfer,photons)
Further reading:
https://en.wikipedia.org/wiki/Spontaneous_emission
https://en.wikipedia.org/wiki/Stimulated_emission
https://en.wikipedia.org/wiki/Emission_spectrum
https://eng.libretexts.org/Bookshelves/Electrical_Engineering/Electro-Optics/Direct_Energy_(Mitofsky)/07%3A_Lamps%2C_LEDs%2C_and_Lasers/7.01%3A_Absorption%2C_Spontaneous_Emission%2C_Stimulated_Emission
https://home.ifa.hawaii.edu/users/kud/teaching_12/5_Atomic_radiation_processes.pdf

Referenced by pages:
21-cm line
absorption
active galactic nucleus (AGN)
active galaxy
advection dominated accretion flow (ADAF)
airglow
alpha CO (αCO)
anomalous microwave emission (AME)
Archeops
ASPECS
atmospheric model
Be star
bolometric magnitude (Mbol)
bremsstrahlung
broad line region (BLR)
circumstellar disk
CMB anisotropies
continuum emission
cooling flow
cooling function
cosmic dust
cosmic microwave background (CMB)
COSMOSOMAS
cyclotron radiation
damping profile
dark matter (DM)
Dickel-Wendker-Bieritz Catalog (DWB)
diffuse emission
Doppler broadening
DQ Tau
DustEM
Dwingeloo Obscured Galaxy Survey (DOGS)
earthshine
Einstein coefficients
electron orbital
electron scattering
electron shell
emission coefficient (j)
emission line
emission line galaxy (ELG)
emission nebula
equation of radiative transfer (RTE)
Europa Clipper
fluorescence
free streaming
Galactic All-sky Survey (GASS)
GALEX Arecibo SDSS Survey (GASS)
gamma rays (GR)
gamma-ray burst (GRB)
gray body
greenhouse effect
Hanle effect
HI Jodrell All-Sky Survey (HIJASS)
HIPASS
hyperluminous infrared galaxy (HLIRG)
intensity mapping (IM)
IRAS 13224-3809
isophote
K-line
Kelvin-Helmholtz mechanism (KH mechanism)
Kirchhoff's law of thermal radiation
limb
line blanketing
line broadening
LINER
long gamma-ray burst (LGRB)
luminosity (L)
luminous infrared galaxy (LIRG)
Lyman-alpha blob
Lyman-break galaxy (LBG)
Lyman-Werner photon
magnetar
magnetic field
maser
Massive Cluster Survey (MACS)
microchannel array
MOJAVE
narrow line region (NLR)
natural broadening
nebula
NEO Surveyor
neutron star (NS)
non-thermal emission
obscured fraction-luminosity relation
OH/IR source
P Cygni profile
PAH emissions
photodissociation
photon
pulsar (PSR)
quantum number
radiation zone
radiative transfer (RT)
radiative transfer code (RT code)
radiative transfer model (RTM)
radio galaxy (RG)
radio supernova (RSN)
random walk
recombination
redshift (z)
retrograde accretion
scattering
secondary eclipse
self-absorption
spectral band
spectral index (α)
spectral line
spectral signature
spectral type
spin-down luminosity
spinning dust emission
standard model of a flare
state of excitation
stellar flare
stimulated emission
synchrotron radiation
thermal bremsstrahlung
thermal dust emission
thermal emission
time-ordered data (TOD)
TIMED
transit spectroscopy
ultra-fast outflow (UFO)
ultraluminous infrared galaxy (ULIRG)
X-ray
X-ray burster (XRB)

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