Wave-Particle Interactions in Astrophysical Plasmas

• Published in: Galaxies Vol. 12; no. 3; p. 28
• Main Author: Pérez-De-Tejada, Héctor
• Format: Journal Article
• Language: English
• Published: Basel MDPI AG 01.06.2024
• Subjects: Black holes; Charged particles; Comets; Conduction heating; Conductive heat transfer; Dissipative processes in transport coefficients; Extrasolar planets; Fluid dynamics; Fluid flow; Heat; Ionosphere; Kinematics; Kinetic theory; Magnetic fields; Mars atmosphere; Mars ionosphere; Mean free path; Momentum; Momentum transport; Particle interactions; Planetary environments; Planetary ionospheres; Planetary magnetic fields; Plasma; Plasma heating; Plasma interactions; Plasma wakes in astrophysics; Shear viscosity; Solar magnetic field; Solar wind; Solar wind magnetic fields; Solar wind particles; Stellar winds; Transport coefficients in plasmas; Upper ionosphere; Venus; Venus ionosphere; Viscosity; Vortex structures in planetary wakes; Wakes; Wave-particle interactions
• ISSN: 2075-4434; 2075-4434
• DOI: 10.3390/galaxies12030028

Dissipation processes derived from the kinetic theory of gases (shear viscosity and heat conduction) are employed to examine the solar wind that interacts with planetary ionospheres. The purpose of this study is to estimate the mean free path of wave-particle interactions that produce a continuum response in the plasma behavior. Wave-particle interactions are necessary to support the fluid dynamic interpretation that accounts for the interpretation of various features measured in a solar wind–planet ionosphere region; namely, (i) the transport of solar wind momentum to an upper ionosphere in the presence of a velocity shear, and (ii) plasma heating produced by momentum transport. From measurements conducted in the solar wind interaction with the Venus ionosphere, it is possible to estimate that in general terms, the mean free path of wave-particle interactions reaches λH ≥ 1000 km values that are comparable to the gyration radius of the solar wind particles in their Larmor motion within the local solar wind magnetic field. Similar values are also applicable to conditions measured by the Mars ionosphere and in cometary plasma wakes. Considerations are made in regard to the stochastic trajectories of the plasma particles that have been implied from the measurements made in planetary environments. At the same time, it is as possible that the same phenomenon is applicable to the interaction of stellar winds with the ionosphere of exoplanets, and also in regions where streaming ionized gases reach objects that are subject to rotational motion in other astrophysical problems (galactic flow–plasma interactions, black holes, etc.).