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Title: |
Measurement and interpretation of magnetic shear in solar active regions
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Author(s): |
Hagyard, M. J.; Rabin, D. M.
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Abstract: |
In this paper a summary and synthesis are presented for results on the role of magnetic shear in the flare process that have been derived from the series of Flare Buildup Study Workshops in the Solar Maximum Analysis program. With emphasis on observations, the mechanisms that seem to produce the sheared magnetic configurations observed in flaring active regions are discussed. The spatial and temporal correlations of this shear with the onset of solar flares are determined from quantitative analyses of measurements of the vector magnetic field. The question of why some areas of sheared magnetic fields are the sites of flares and others are not is investigated observationally.
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NASA Center: |
Marshall Space Flight Center
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Publication Date: |
JAN 1, 1986
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Document Source: |
Other Sources |
No Digital Version Available: |
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Document ID: |
19870052703
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Accession ID: |
87A39977
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Publication Information: |
Advances in Space Research, 6, 6, 19, 7-16, ISSN 0273-1177, Number of Pages = 10 |
Related Information: |
NASA-USAF-supported resear |
Keywords: |
MAGNETOHYDRODYNAMIC SHEAR HEATING; SOLAR ACTIVITY; SOLAR FLARES; SOLAR MAGNETIC FIELD;
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Notes: |
(COSPAR, SCOSTEP, and IAU, Plenary Meeting, 26th, Symposium on the Physics of Solar Flares, 5th, Toulouse, France, June 30-July 11, 1986) Advances in Space Research (ISSN 0273-1177), vol. 6, no. 6, 1986, p. 7-16. NASA-USAF-supported research. |
Accessibility: |
Unclassified; Copyright; Unlimited; Publicly available; |
Updated/Added to NTRS: |
2004-11-03 |
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