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Title: |
Quiet-Region Filament Eruptions
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Author(s): |
Choudhary, Debi Prasad; Moore, Ronald L.
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Abstract: |
We report characteristics of quiescent filament eruptions that did not produce coronal mass ejections (CMEs). It is known that there is a dichotomy of quiescent filament eruptions: those that produce CMEs and those that do not. We examined the quiescent filament eruptions, each of which was located far from disk center (greater than or equal to 0.7 R(sub Sun)) in diffuse remnant magnetic fields of decayed active regions, was well observed in Ha observations and Fe XII, and had good coronagraph coverage. We present the similarity and differences of two classes of filament eruptions. From their lack of CME production and the appearance of their eruptive motion in Fe XII movies, we conclude that the non-CME-producing filament eruptions are confined eruptions like the confined filament eruptions in active regions. We take the similarity of the confined and eruptive quiescent filament eruptions with their active-region counterparts to favor runaway tether-cutting connection for unleashing the magnetic explosion in all these eruptions.
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NASA Center: |
Marshall Space Flight Center
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Publication Date: |
[2004]
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Document Source: |
Other Sources |
No Digital Version Available: |
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Available Data: |
Abstract Only |
Document ID: |
20040082298
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Publication Information: |
Number of Pages = 1 |
Meeting Information: |
204th Meeting of the American Astronomical Society, 30 May - 3 Jun. 2004, Denver, CO, United States |
Keywords: |
CORONAL MASS EJECTION; DICHOTOMIES; SOLAR PROMINENCES; GEOPHYSICS; MAGNETIC FIELDS; SUN; H ALPHA LINE; CORONAGRAPHS;
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Accessibility: |
Unclassified; No Copyright; Unlimited; Publicly available; |
Updated/Added to NTRS: |
2004-10-28 |
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