Waves and instabilities in the solar wind

Journal Article · Sat Feb 01 04:00:00 EST 1975 · Rev. Geophys. Space Phys., v. 13, no. 1, pp. 263-289

DOI:https://doi.org/10.1029/RG013i001p00263· OSTI ID:4159535

Hollweg, J V

We present a review of waves and instabilities in the solar wind, concentrating on those aspects that are likely to play important roles in influencing the dynamic and thermodynamic states of the general solar wind expansion. We consider in particular the roles played by various waves and instabilities in influencing the heating and expansion of the solar wind, the angular momentum of the solar wind, the solar wind thermal anisotropy, the heating and flow of alpha particles in the solar wind, the interstellar neutral particles that become ionized in the solar wind, and the ''fluidlike behavior'' of the solar wind. We include a brief review of the properties of the hydromagnetic wave modes, concentrating particularly on the Alfven mode, which has been observed to contribute significantly to the microscale fluctuations of the solar wind. But we also present a summary of observational evidence pertaining to the presence and action in the solar wind of waves and instabilities that are not among the hydromagnetic modes. (auth)

• Research Organization: National Center for Atmospheric Research, Boulder, CO
• Sponsoring Organization: USDOE
• NSA Number: NSA-33-001707
• OSTI ID: 4159535
• Journal Information: Rev. Geophys. Space Phys., v. 13, no. 1, pp. 263-289, Journal Name: Rev. Geophys. Space Phys., v. 13, no. 1, pp. 263-289; ISSN RGPSB
• Country of Publication: United States
• Language: English

Related Subjects

*SOLAR WIND-- WAVE PROPAGATION
640107* --Physics Research--Astrophysics & Cosmology-- Planetary Phenomena
ALPHA PARTICLES
ANGULAR MOMENTUM
ANISOTROPY
EXPANSION
FLUCTUATIONS
HEATING
HYDRODYNAMIC MODEL
INTERSTELLAR GRAINS
IONIZATION
N56700* --Physics (Astrophysics & Cosmology)--Planetary Phenomena