X-ray emission from seventeen X-ray flares was analyzed to obtain electron temperatures and emission measures associated with the source region in the solar corona. The source region was assumed to be isothermal with a Maxwellian electron velocity distribution. Flares which were characterized by a
The time behavior of temperature and emission measure in X-ray flares
โ Scribed by Robert W. Milkey; Norman K. Blocker; William H. Chambers; Paul E. Fehlau; Jack C. Fuller; Walter E. Kunz
- Publisher
- Springer
- Year
- 1971
- Tongue
- English
- Weight
- 551 KB
- Volume
- 20
- Category
- Article
- ISSN
- 0038-0938
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