Magnetic reconnection in the solar atmosphere

被引：0
|
作者：
Somov, BV
机构：
来源：
ICPP 96 CONTRIBUTED PAPERS - PROCEEDINGS OF THE 1996 INTERNATIONAL CONFERENCE ON PLASMA PHYSICS, VOLS 1 AND 2 | 1997年
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中图分类号：
T [工业技术];
学科分类号：
08 ;
摘要：
Observations with the hard and soft X-ray telescopes on board Yohkoh show that reconnection is responsible for many non-steady phenomena in the solar atmosphere. The reconnection theory - more exactly, the model of a high-temperature turbulent-current sheet (HTTCS) - is reviewed in applying to the coronal conditions derived from the Yohkoh data on the site and mechanism of magnetic energy transformation into kinetic and thermal energies of 'super-hot' plasma and accelerated particles.
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页码：498 / 501
页数：4
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