An Observational and Conceptual Model of the Magnetic Field of a Filament

作者: Sara F. Martin , Christopher R. Echols

DOI: 10.1007/978-94-011-1188-1_29

关键词:

摘要: A conceptual, scale model of the geometry magnetic field a filament was developed primarily from: (1) observed structure recorded in H-alpha filtergrams, (2) calculations height (3) association appendages along sides with patches photospheric flux opposite polarity to network fields on each side filament, (4) ends and (5) assumption that fine is parallel filament. The consistent inverse category quiescent prominences. three-dimensional sufficiently simple wire used represent imaginary lines their relationship magnetogram.

参考文章(7)
Solar photosphere: Structure, convection and magnetic fields Proceedings of the 138th International Astronomical Union (IAU) Symposium. ,(1989) , 10.1007/978-94-009-1061-4
Peter Foukal, Morphological relationships in the chromospheric H? fine structure Solar Physics. ,vol. 19, pp. 59- 71 ,(1971) , 10.1007/BF00148824
G. A. Gary, R. L. Moore, M. J. Hagyard, Bernhard M. Haisch, Nonpotential features observed in the magnetic field of an active region The Astrophysical Journal. ,vol. 314, pp. 782- ,(1987) , 10.1086/165104