NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
The optical flareA survey is presented of the available information on the flare process contained in optical observations. It is shown that the flare process is always associated with filaments and with the simplification of existing magnetic connections. The flare process also arises from the emergence and expansion of new flux. The optical flare can be divided into the impulsive phase, in which multiple flashes along the neutral line are exhibited, and the thermal phase, in which two-ribbon expansion is present. It is shown that the impulsive phase resembles tearing mode phenomena. Very high densities in these phenomena are required by the appearance of loops in emission. Several unanswered questions relating to the flare process are examined, including the ratios of the hydrogen lines, the excitation of He II 4686, and the relation of the vertical to the horizontal structures.
Document ID
19830066457
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Zirin, H.
(Big Bear Solar Observatory Pasadena, CA, United States)
Date Acquired
August 11, 2013
Publication Date
July 1, 1983
Publication Information
ISSN: 0038-0938
Subject Category
Solar Physics
Report/Patent Number
ISSN: 0038-0938
Accession Number
83A47675
Funding Number(s)
CONTRACT_GRANT: NSF ATM-81-12698
CONTRACT_GRANT: NGL-05-002-034
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available