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Predicting the Sign of Magnetic Helicity in Erupting Filaments and Coronal Mass Ejections

2011; American Geophysical Union; Linguagem: Inglês

10.1029/gm099p0127

2328-8779

S. F. Martin, A. H. McAllister,

Astro and Planetary Science

Predicting the Sign of Magnetic Helicity in Erupting Filaments and Coronal Mass Ejections S. F. Martin, S. F. Martin Helio Research, 5212 Maryland Ave., La Crescenia, CaliforniaSearch for more papers by this authorA. H. McAllister, A. H. McAllister High Altitude Observatory, PO Box 3000, Boulder, ColoradoSearch for more papers by this author S. F. Martin, S. F. Martin Helio Research, 5212 Maryland Ave., La Crescenia, CaliforniaSearch for more papers by this authorA. H. McAllister, A. H. McAllister High Altitude Observatory, PO Box 3000, Boulder, ColoradoSearch for more papers by this author Book Editor(s):Nancy Crooker, Nancy CrookerSearch for more papers by this authorJo Ann Joselyn, Jo Ann JoselynSearch for more papers by this authorJoan Feynman, Joan FeynmanSearch for more papers by this author First published: 01 January 1997 https://doi.org/10.1029/GM099p0127Citations: 40Book Series:Geophysical Monograph Series AboutPDFPDF ToolsRequest permissionExport citationAdd to favoritesTrack citation ShareShareShare a linkShare onEmailFacebookTwitterLinkedInRedditWechat Summary This chapter contains sections titled: Introduction Geometric Properties of Erupting Coronal Arcades Geometric Properties of Erupting Filaments Summary References S. K. Antiochos, R. B. Dahlburg, J. A. Klimchuk, The magnetic field of solar prominences, Astrophys. J., 420, L41– L44, 1994. 10.1086/187158 Web of Science®Google Scholar V. Bothmer, and D. M. 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