The observational difficulties of obtaining the magnetic field distribution in the chromosphere and corona of the Sun has led to methods of extending photospheric magnetic measurements into the solar atmosphere by mathematical procedures. A new approach to this problem presented here is that a const
Solar magnetic cycle: Peculiarities of the photospheric field distribution
โ Scribed by E. S. Vernova; M. I. Tyasto; D. G. Baranov
- Book ID
- 110164066
- Publisher
- SP MAIK Nauka/Interperiodica
- Year
- 2009
- Tongue
- English
- Weight
- 132 KB
- Volume
- 49
- Category
- Article
- ISSN
- 0016-7932
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