Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...390..560c&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 390, no. 2, May 10, 1992, p. 560-566.
Astronomy and Astrophysics
Astrophysics
17
Compressibility, Magnetohydrodynamic Waves, Wave Attenuation, Wave Propagation, Analytic Functions, Magnetosonic Resonance, Mathematical Models, Propagation Modes, Shear
Scientific paper
The effect of compressibility on the propagation and resistive dissipation properties of magnetohydrodynamic waves in nonuniform media is studied by using a normal mode analysis. The paper concentrates on wave models for which the resistivity acts over the entire system, thus excluding localized resonant absorption. The wave modes in nonhomogeneous situations are identified in term of their familiar homogeneous counterparts and it is shown that only the shear Alfven and slow magnetosonic modes survive in the resistive regime. The most promising heating agents in the astrophysical context are shown to be the shear Alfven waves that behave almost incompressibly.
Califano Francesco
Chiuderi Claudio
Einaudi Giorgio
No associations
LandOfFree
Nonresonant resistive dissipation of compressible magnetohydrodynamic waves does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Nonresonant resistive dissipation of compressible magnetohydrodynamic waves, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Nonresonant resistive dissipation of compressible magnetohydrodynamic waves will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1514709