Intensities and profiles of the Ha, H/3, H3,, K, and D3 lines are measured in a solar prominence. From the profiles of these lines we estimate T = 6400 K and vt = 5.7 km s -1. We construct a simple isothermal model which explains the Ha intensity and profile for an assumed total particle density nT
โฆ LIBER โฆ
A spectral model based on atmospheric self-memorization principle
โ Scribed by Xiangqian Gu
- Publisher
- Springer
- Year
- 1998
- Tongue
- English
- Weight
- 576 KB
- Volume
- 43
- Category
- Article
- ISSN
- 1001-6538
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