Astrophysics (Index)About

plasma

(state of matter in which atoms are separate and ionized)

Plasma is a state of matter in addition to solid, liquid, and gas. Plasma is gas-like but the atoms are free of molecular bonds and a significant number are ionized. A body of plasma typically includes both positive and negative particles, e.g., ions, electrons, and positrons usually balanced so that the body as a whole is neutral. The threshold distinguishing plasma from gas (i.e., "how much of the material needs to be ionized?") has no universally-used precise definition, but generally reflects the notion that a gas is plasma if it shows distinct qualities of plasma, such as electrical conductivity and interaction with magnetic fields.

The plasma state is maintained by high temperature. Stars such as the Sun are sufficiently hot as to ionize much of their matter, much of the interstellar medium (ISM) is ionized and the intergalactic medium through galaxy clusters is generally highly ionized. Though plasma is rare on Earth, the vast majority of the universe's baryonic matter is plasma.

Plasma is used in technology such as neon signs and plasma displays.

Collisionless plasma is plasma which lack the constant collisions between particles found in a (neutral) gas, i.e., particles passing so close that their directions are decidedly changed. Rather the particles' movements, under the influence of the fields and plasma waves, are not random and such collisions are relatively rare or non-existent. This is common in the low density of the ISM, for example.


(physics)
Further reading:
https://en.wikipedia.org/wiki/Plasma_(physics)
https://en.wikipedia.org/wiki/Astrophysical_plasma
http://hyperphysics.phy-astr.gsu.edu/hbase/Chemical/plasma.html
https://dictionary.obspm.fr/index.php?formSearchTextfield=plasma&showAll=1
https://www.psfc.mit.edu/vision/what_is_plasma
https://arxiv.org/abs/1404.0509
https://www.astro.princeton.edu/~kunz/Site/AST521/AST521_lecture_notes_Kunz.pdf
https://physics.stackexchange.com/questions/535679/differences-between-cold-and-collisionless-plasma

Referenced by pages:
21-cm experiment
active galactic nucleus (AGN)
Aditya-L1
Alfvén wave (AW)
baryon acoustic oscillations (BAO)
beta (β)
black-body radiation
Bose-Einstein condensate (BEC)
BPT diagram
bremsstrahlung
Bullet Cluster
Cassini
chemodynamics
CHIPS
chondrite
Cloudy
collisional broadening
comet
Compton scattering
cooling flow
corona
coronal hole
coronal loop
coronal mass ejection (CME)
current sheet
Debye length
Deep Space 1 (DS1)
degree of ionization
diffuse emission
diffusion damping
DISCOVR
electron (e-)
electron pressure
electron screening
electron volt (eV)
equation of radiative transfer (RTE)
Europa Clipper
Faraday rotation
filament
fluorescence
flux freezing
fossil group
Güdel-Benz relation
GADGET-2
galactic halo
galaxy cluster (CL)
Galileo
gas flow
Giotto
gravitomagnetic field
Hall effect
Herbig-Haro object (HH)
IMAGE­
intergalactic medium (IGM)
International Cometary Explorer (ICE)
interplanetary medium (IPM)
intracluster medium (ICM)
Io
ion
jet
jet current
Juno
kappa distribution
Landau damping
Langmuir probe (LP)
Lorentz force
Mach number
magnetic energy spectrum
magnetic field
magnetic reconnection
magnetohydrodynamics (MHD)
magnetosonic wave
Magnetospheric Multiscale Mission (MMS)
Mars Express
MESSENGER
microwave
Ohmic heating
partial ionization zone
phase transition
photosphere
PIC simulation
Pioneer Venus Orbiter (PVO)
planetary nebula (PN)
plasma astrophysics
plasma frequency
plasma wave
plasmon
quantum tunneling
quark-gluon plasma (QGP)
quasiparticle
radiative transfer (RT)
radiative transfer code (RT code)
radio phoenix
radio relics
reverberation mapping
Reynolds number (Re)
Rosetta
Rosseland mean opacity
Saha equation
scintillometry
SELENE
shock wave
Solar Orbiter (SolO)
source function (S)
standard model of a flare
Stark effect
stellar atmosphere
stellar model atmosphere
STEREO
Sun surface features
Sunyaev-Zel'dovich effect (SZ effect)
supershell
suprathermal
surface of last scattering
surface temperature
SWFO-L1
thermal bremsstrahlung
thermal emission
Ulysses
Uranus Orbiter and Probe
Venus Express
Vlasov-Poisson equation
vortex
Voyager
Wind
X-ray source

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