Solar millisecond spikes manifest large-and small-scale inhomogeneities of the coronal plasma
| Autor: | V. G. Vlasov, A. A. Kuznetsov |
|---|---|
| Rok vydání: | 2003 |
| Předmět: |
Physics
Millisecond Cyclotron resonance Astronomy and Astrophysics Plasma Radiation Electron cyclotron resonance Computational physics law.invention Magnetic field Physics::Plasma Physics Space and Planetary Science law Physics::Space Physics Astrophysics::Solar and Stellar Astrophysics Energy transformation Maser Atomic physics |
| Zdroj: | Astronomy Reports. 47:129-138 |
| ISSN: | 1562-6881 1063-7729 |
| DOI: | 10.1134/1.1554516 |
| Popis: | A model for the generation of solar millisecond radio spikes via a maser cyclotron resonance is proposed. The model takes into account the large-scale inhomogeneity of the magnetic field and small-scale inhomogeneities of the coronal plasma. The efficiency of the energy transformation from a electron beam into maser radiation is estimated. Appropriate parameters of the magnetic field inhomogeneity and the plasma turbulence are found. |
| Databáze: | OpenAIRE |
| Externí odkaz: |
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