The Hard X-ray Imaging Spectrometer aboard the SMM detected gigantic arches in the corona which are formed or, if preexisting, become excited after major two-ribbon flares. They are seen in 3.5-8 keV X-rays and extend along the Hjl = 0 line to altitudes between l0 s and 2 x 105 km. These arches are
Thermal structures associated with post-flare coronal arches
✍ Scribed by Paul Hick; Zdeněk Švestka
- Publisher
- Springer
- Year
- 1987
- Tongue
- English
- Weight
- 1011 KB
- Volume
- 108
- Category
- Article
- ISSN
- 0038-0938
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