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The two types of flare associated filament eruptionsUsing years of high resolution solar footage obtained at Big Bear Solar Observatory flare associated filament eruptions were studied. In addition to the classical type eruption consisting of expansion and breakup, evidence was found of another type where a layer is shed from the filament and erupts while the inversion line filament below (or, what is left of it) remains in place. Both types of eruptions are presented. It is hoped that the new evidence will shed new light on the understanding of the role of filaments in flares.
Document ID
19860012015
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Tang, F.
(California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
September 5, 2013
Publication Date
January 1, 1986
Subject Category
Solar Physics
Report/Patent Number
NASA-CR-176571
NAS 1.26:176571
BBSO-0255
Accession Number
86N21486
Funding Number(s)
CONTRACT_GRANT: NGL-05-002-034
CONTRACT_GRANT: NSF ATM-85-13577
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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