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- W2000393208 abstract "view Abstract Citations (36) References (17) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Electron heating by fast mode magnetohydrodynamic waves in the solar wind emanating from coronal holes Habbal, S. R. ; Leer, E. Abstract It is shown that fast mode magnetohydrodynamic waves, propagating outwards from the sun in coronal hole regions, will dissipate primarily through collisionless interaction with electrons rather than with protons. This dissipation can lead to higher electron than proton temperatures in the accelerating region of the solar wind, provided the waves carry a sufficiently large energy flux. Publication: The Astrophysical Journal Pub Date: February 1982 DOI: 10.1086/159637 Bibcode: 1982ApJ...253..318H Keywords: Coronal Holes; Electron Energy; Magnetohydrodynamic Waves; Plasma-Particle Interactions; Propagation Modes; Solar Wind; Collisionless Plasmas; Energy Dissipation; Proton Energy; Radiant Flux Density; Solar Physics full text sources ADS |" @default.
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- W2000393208 title "Electron heating by fast mode magnetohydrodynamic waves in the solar wind emanating from coronal holes" @default.
- W2000393208 doi "https://doi.org/10.1086/159637" @default.
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