Solar coronal heating by magnetosonic waves
✍ Scribed by E.R. Pekünlü; Ö. Çakırlı; E. Özetken
- Publisher
- John Wiley and Sons
- Year
- 2001
- Tongue
- English
- Weight
- 146 KB
- Volume
- 326
- Category
- Article
- ISSN
- 0035-8711
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📜 SIMILAR VOLUMES
## Abslrar -k quantJtallxc ,,tud.~ Js made based on the suggeslion that coronal heating results from I.andau damping of ion acoustic x~axcs, h is sho~n that both ions and electrons are heated by mmhnear >aluralion of loll acoustic instabilitx, hms are heated more rapidb 111::111 the electrons.
We have modeled the solar coronal active loop heating by discrete Alfv6n waves. Discrete Alfv~n waves (DAW) are a new class of Alfv6n waves which can be described by the two-fluid model with finite ion-cyclotron frequency, or the MHD model with plasma current along the magnetic field line as shown b