Although the Ca II K232 network is known to be cospatial with magnetic elements there has been doubt as to the magnetic origin of the fainter Kzv points. We demonstrate that weak magnetic elements also lie at the roots of the K2v points, and because the latter are numerous they may contribute sensib
โฆ LIBER โฆ
Observations of Photospheric Dynamics and Magnetic Fields: From Large-Scale to Small-Scale Flows
โ Scribed by N. Meunier; J. Zhao
- Publisher
- Springer Netherlands
- Year
- 2008
- Tongue
- English
- Weight
- 909 KB
- Volume
- 144
- Category
- Article
- ISSN
- 0038-6308
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