h is shown by using a 3-D resislive MI ID simulation code, taking inlo account the recombination effect, that magnetic reconnection during collision o[ txvo current loops can be enhanced by lccombination. It is also shown that lhe temperature in the thin current sheet formed between two loops increa
โฆ LIBER โฆ
Classification of magnetic reconnection during two current-loop coalescence
โ Scribed by Jun-ichi Sakai; Shinji Koide
- Book ID
- 104643920
- Publisher
- Springer
- Year
- 1992
- Tongue
- English
- Weight
- 421 KB
- Volume
- 142
- Category
- Article
- ISSN
- 0038-0938
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โฆ Synopsis
We present a classification of magnetic reconnection during two current loop coalescence, which may be quite important for the physical process of both solar flares and coronal loop heating in the solar active region. It is suggested that different kinds of the current loop coalescence processes could be identified from the soft X-ray telescope(SXT ) of the " Yohkoh " satellite and the magnetic field data in the active region.
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