Very bright and highly circularly polarized radio bursts from the Sun, the planets, flare stars, and close binary stars are attributed to the electron-cyclotron maser instability. The mode and frequency of the dominant radiation from the maser instability is shown to be dependent on the plasma tempe
β¦ LIBER β¦
Evidence for cyclotron maser emission from the Sun and stars
β Scribed by G. A. Dulk; R. M. Winglee
- Publisher
- Springer
- Year
- 1987
- Tongue
- English
- Weight
- 366 KB
- Volume
- 113
- Category
- Article
- ISSN
- 0038-0938
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β¦ Synopsis
In recent years radiation has been observed from planets, Sun and stars that is best explained by the cyclotron maser instability; in fact, all celestial bodies that might feasibly emit and be detected by their cyclotron maser radiation have been detected.
Here we review those observations, the developments in the theory, the recent work on the e~ency of energy transfer by cyclotron maser radiation, and some recent and future observations that might demonstrate whether the mechanism is energetically important in solar and stellar flares.
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