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Magnetic Reconnection in the Solar Lower Atmosphere
2002ABSTRACT There are many active phenomena, such as Ellerman bombs (EBs), Type II white-light flares (WLFs) etc, appear in the solar lower atmosphere. They have many common features despite of the large energy gap between them. They are considered to result from the local heating in the solar lower atmosphere.
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Evidence of Magnetic Reconnection in Solar Flares
1996The detailed analysis of the 1992 February 21 flare indicates that magnetic reconnection is responsible for heating of the thermal plasmas produced in the flare. The plasma density enhancement presumably associated with slow shocks is observed. The Yohkoh observations of this flare fit well with the Petschek model, and the structure of the slow shock ...
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Magnetic Reconnection in Solar Flares [Slides]
2023Teresa Boland, Fan Guo, Timothy Waters
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Prevalence of magnetic reconnection at small field shear angles in the solar wind
Geophysical Research Letters, 2007Adam Szabó, J T Gosling
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Impulsive Magnetic Reconnection in the Earth's Magnetotail and the Solar Corona
Annual Review of Astronomy and Astrophysics, 2004Amitava Bhattacharjee
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Solar wind control of the radial distance of the magnetic reconnection site in the magnetotail
Journal of Geophysical Research, 2005Wolfgang Baumjohann +2 more
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