A re-analysis of the brightness distribution of the quiet Sun at 1.2 mm wavelength is made. It is concluded that there is no evidence for uniform or limb-brightened distribution at this wavelength. \* NAS-NRC Research Associate on sabbatical leave from the University of Maryland.
Compact, variable sources on the Sun at 2 centimeter wavelength
โ Scribed by Robert F. Willson; Kenneth R. Lang
- Publisher
- Springer
- Year
- 1988
- Tongue
- English
- Weight
- 882 KB
- Volume
- 114
- Category
- Article
- ISSN
- 0038-0938
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โฆ Synopsis
Very Large Array (VLA) observations of compact transient sources on the Sun at 2 cm wavelength are presented. These sources have angular sizes of 0~5"-25", brightness temperatures of T~ ~ 1-3 x 105 K, and lifetimes ranging between a few minutes to several hours. The emission originates in regions of diffuse plage and quiet Sun, where the photospheric magnetic fields are relatively weak (H < 100 G). In some cases the 2 cm radiation may be explained as the thermal bremsstrahlung of a dense (Are < 101~ cm-3) plasma in the transition region. For other sources, the relatively high circular polarization (Pc ~ 40-50 %) suggests a nonthermal emission mechanism, such as the gyrosynchrotron radiation of mildly relativistic electron with a power-law spectrum.
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