The temperature and density are obtained for coronal plasma in thermal and hydrostatic equilibrium and located in a force-free magnetic arcade. The isotherms are found to be inclined to the magnetic field lines and so care should be taken in inferring the magnetic structure from observed emission.
✦ LIBER ✦
“Dawn-dusk asymmetry” in solar coronal arcade formations
✍ Scribed by Isobe, Hiroaki
- Book ID
- 118663483
- Publisher
- American Geophysical Union
- Year
- 2002
- Tongue
- English
- Weight
- 212 KB
- Volume
- 29
- Category
- Article
- ISSN
- 1944-8007
No coin nor oath required. For personal study only.
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