Coronal Heating: Energy Release Associated with Chromospheric Magnetic Reconnection

2000 ◽  
Vol 538 (2) ◽  
pp. 960-967 ◽  
Author(s):  
Colin B. Roald ◽  
P. A. Sturrock ◽  
Richard Wolfson
Keyword(s):  
Magnetic Reconnection ◽  
Energy Release ◽  
Coronal Heating

Magnetic reconnection and energy release in a long-duration stellar flare

1986 ◽  
Vol 6 (8) ◽  
pp. 145-148 ◽  
Author(s):  
G. Poletto ◽  
R. Pallavicini ◽  
R.A. Kopp
Keyword(s):  
Magnetic Reconnection ◽  
Energy Release ◽  
Stellar Flare ◽  
Long Duration

Possible two-step solar energy release mechanism due to turbulent magnetic reconnection

2005 ◽  
Vol 12 (5) ◽  
pp. 052901 ◽  
Author(s):  
Quan-Lin Fan ◽  
Xue-Shang Feng ◽  
Chang-Qing Xiang
Keyword(s):  
Solar Energy ◽  
Magnetic Reconnection ◽  
Energy Release ◽  
Release Mechanism

Chromospheric Magnetic Reconnection and its Implication for Coronal Heating

1999 ◽  
Vol 524 (1) ◽  
pp. L75-L78 ◽  
Author(s):  
P. A. Sturrock ◽  
C. B. Roald ◽  
R. Wolfson
Keyword(s):  
Magnetic Reconnection ◽  
Coronal Heating

scholarly journals Hard X-ray Spectrum of the Above-the-Looptop Source in Impulsive Solar Flares

2000 ◽  
Vol 195 ◽  
pp. 413-414
Author(s):  
S. Masuda
Keyword(s):  
Magnetic Reconnection ◽  
Energy Release ◽  
Solar Flares ◽  
Count Rate ◽  
High Quality ◽  
X Ray ◽  
Flare Energy

Extended AbstractThe Hard X-ray Telescope (HXT: Kosugi et al. 1991) onboard Yohkoh has observed that, in impulsive solar flares, a hard X-ray source is located above the apex of a soft X-ray flaring loop, in addition to double footpoint sources (Masuda et al. 1994, 1995). This observation suggests that flare energy-release, probably magnetic reconnection, takes place not in the soft X-ray loop but above the loop. It is important to derive the hard X-ray spectrum of the above-the-looptop source accurately in order to understand how electrons are energized there. The above-the-looptop source was most clearly observed during the 13 January 1992 flare. However, the count rate, especially in the H-band (53–93 keV), is too small to synthesize high-quality images and to derive an accurate spectrum.

scholarly journals The role of compressibility in energy release by magnetic reconnection

2012 ◽  
Vol 19 (8) ◽  
pp. 082109 ◽  
Author(s):  
J. Birn ◽  
J. E. Borovsky ◽  
M. Hesse
Keyword(s):  
Magnetic Reconnection ◽  
Energy Release
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