interplanetary medium
(IPM)
(matter in the solar system around and between planets)
The interplanetary medium (IPM) is matter such as dust,
gas, and plasma within the solar system between planets.
The plasma is solar wind, a substantial part of the IPM. IPM
density varies, generally thinner away from the Sun (a steady
solar wind would decrease in density according to an
inverse square law).
The density at 1 AU (i.e., the vicinity of Earth) is on
the order of 5 particles per cubic centimeter. Given the
electrically-conducting plasma, a magnetic field is maintained,
forming a dynamo. The dust,
known as interplanetary dust particles (IDP), is generally dust
fragments of asteroids, etc.
Analogous matter between stars is called the interstellar medium
and between galaxies, the intergalactic medium.
(gas,dust,solar system)
Further reading:
https://en.wikipedia.org/wiki/Interplanetary_medium
https://targetstudy.com/nature/solar-system/interplanetary-medium/
https://www.britannica.com/science/interplanetary-medium
https://en.wikiversity.org/wiki/Interplanetary_medium
https://nineplanets.org/the-interplanetary-medium/
http://astroa.physics.metu.edu.tr/nineplanets/medium.html
https://web.njit.edu/~gary/320/Lecture24.html
Referenced by pages:
2175 angstrom feature
airglow
circumstellar envelope (CSE)
cosmic dust
foreground subtraction
magnetohydrodynamics (MHD)
mass density
particle spectrometer
plasma frequency
plasma wave
presolar grain
refraction
scintillometry
shock wave
sky subtraction
solar system
Stardust
stellar atmosphere
Index