Non-inductive current driven by Alfvén waves in solar coronal loops
✍ Scribed by A. G. Elfimov; C. A. Azevedo; A. S. Assis
- Publisher
- Springer
- Year
- 1996
- Tongue
- English
- Weight
- 768 KB
- Volume
- 167
- Category
- Article
- ISSN
- 0038-0938
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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
It is shown that a discrete Alfv6n wave can explain the natural oscillations of solar loop prominences by considering the existence of a current flow. Discrete Alfv6n waves are a new class of Alfv6n waves which is described by the inclusion of the finite ion cyclotron frequency (e)/e)~i ~ 0) and/or