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The electron density in clouds of turbulent interstellar plasma

Astronomy Reports, 2016
The dependence of the emission measure on the dispersion measure due to the Galactic background has been derived for 120 directions in the Galaxy. This analysis has yielded the mean electron density, effective thickness of the electron layer, and the volume filling factor of the clouds of ionized gas along the line of sight.
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Distribution of inhomogeneities in the interstellar plasma in the directions of three distant pulsars from observations with the RadioAstron ground–space interferometer

, 2016
M. Popov   +11 more
semanticscholar   +1 more source

Ionic Processes in Low Temperature Interstellar Molecular Plasmas

AIP Conference Proceedings, 2002
Astrophysical plasmas vary widely in their temperatures and compositions. Some of the most tenuous, coldest, and spatially extensive are the diffuse and dense interstellar clouds, in the latter of which stars are forming. In these regions, including circumstellar shells, ∼130 molecules have been detected with ∼10% being ions.
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A theoretical study of elementary processes in interstellar plasma

Une étude théorique de processus élémentaires dans le plasma interstellaire Le plasma est le plus abondant des états de la matière — les étoiles, le vent solaire, et le milieu interstellaire sont considérés comme des plasmas. Des nuages de gaz et de poussière composant ce dernier sont une première étape importante de la formation des ...
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Plasma velocities in the Heliosheath and the influence of the interstellar wind

2009
A new coordinate system (Interstellar Heliospheric Coordinates, or IHC) is introduced to enable the detailed study of the influence of the interstellar wind on the heliosheath. Recent, in situ measurements of plasma velocities in the heliosheath by Voyager 2 are projected into the IHC system and analyzed.
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