Research output per year
Research output per year
Project Details
Description
The propagation of ideal MHD waves in half spaces separated by a current sheet is studied. Local dissipation within the current layer generates magnetic reconnection which acts as a source for plasma waves. A mathematical model for the nonlinear decay of the current sheet togehter with the linear wave perturbation is set up and investigated analytically as well as numerically.
The results are applied to satellite data from the magnetopause in order to understand the interaction of the solar wind with magnetospheric plasma.
| Status | Finished |
|---|---|
| Effective start/end date | 1/01/94 → 15/09/15 |
Fingerprint
Explore the research topics touched on by this project. These labels are generated based on the underlying awards/grants. Together they form a unique fingerprint.
-
Buoyancy and the Penrose process produce jets from rotating black holes
Semenov, V., Dyadechkin, S. A. & Heyn, M., 2014, In: Physica Scripta. 89, 045003.Research output: Contribution to journal › Article › peer-review
-
Buoyancy of relativistic magnetic flux tubes and Penrose process produce jets from Kerr black holes
Semenov, V., Dyadechkin, S. & Heyn, M., 2014, AIP Conference Proceedings. American Institute of Physics Publising LLC, p. 66-70Research output: Chapter in Book/Report/Conference proceeding › Conference paper › peer-review
Open AccessFile -
Kelvin-Helmholtz stability of reconnection exhausts in the solar wind
Sasunov, Y. L., Semenov, V., Heyn, M., Kubyshkin, I. & Biernat, H., 2012, In: Geophysical Research Letters. 39, p. L06104- L06104Research output: Contribution to journal › Article › peer-review