The formation of shocks and shock heating by radiatively damped longitudinal waves in solar magnetic flux tubes of different filling factors is studied. We consider three flux tubes of filling factors: 1%, 20%, and exponentially spreading which represent normal, enhanced network regions and the inte
โฆ LIBER โฆ
Dependence of the canopy height of solar magnetic flux tubes on its definition
โ Scribed by MEI Zhang; HONGQI Zhang
- Book ID
- 110222411
- Publisher
- Springer
- Year
- 2000
- Tongue
- English
- Weight
- 45 KB
- Volume
- 194
- Category
- Article
- ISSN
- 0038-0938
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