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
✦ LIBER ✦
Simultaneous measurements of X-rays and electrons during a pulsating aurora
✍ Scribed by N. Østgaard; J. Stadsnes; K. Aarsnes; F. Søraas; K. Måseide; M. Smith; J. Sharber
- Book ID
- 106189724
- Publisher
- Copernicus Group
- Year
- 1998
- Tongue
- English
- Weight
- 921 KB
- Volume
- 16
- Category
- Article
- ISSN
- 0992-7689
No coin nor oath required. For personal study only.
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