Previous efforts to construct solar coronal fields using surface magnetograph data have generally employed a least squares minimization technique in order to determine the spherical harmonic expansion coefficients of the magnetic scalar potential. Provided there is no source surface high up in the c
โฆ LIBER โฆ
Direct solution of laplace's equation for coronal magnetic fields using line-of-sight boundary conditions
โ Scribed by W. Riesebieter; F. M. Neubauer
- Publisher
- Springer
- Year
- 1979
- Tongue
- English
- Weight
- 296 KB
- Volume
- 63
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
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