Radiative and conductive cooling in a solar flare
β Scribed by Zongjun Ning; Dong Li
- Publisher
- Springer Netherlands
- Year
- 2011
- Tongue
- English
- Weight
- 477 KB
- Volume
- 338
- Category
- Article
- ISSN
- 0004-640X
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π SIMILAR VOLUMES
Solar flare X-rays, at energies less than 10 keV, are emitted by hot plasmas located in the corona. Three plasma cooling models are examined in detail. The cooling of the electrons by Coulomb collisions with ions at a lower temperature would require the observed material to occupy very large volumes
High temporal and spatial resolution solar X-ray pictures of a flare at 1827 UT on 5 September 1973 were taken with the S-056 Aerospace Corporation/MarshaU Space Flight Center telescope on the Apollo Telescope Mount. Photographs taken at 9 s intervals allow detailed information to be obtained about