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A model for straight and helical solar jets: II. Parametric study of the plasma beta
CONTEXT: Jets are dynamic, impulsive, well-collimated plasma events that develop at many different scales and in different layers of the solar atmosphere. AIMS: Jets are believed to be induced by magnetic reconnection, a process central to many astrophysical phenomena. Within the solar atmosphere, j...
में बचाया:
| में प्रकाशित: | Astron Astrophys Suppl Ser |
|---|---|
| मुख्य लेखकों: | , , , , |
| स्वरूप: | Artigo |
| भाषा: | Inglês |
| प्रकाशित: |
2016
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| विषय: | |
| ऑनलाइन पहुंच: | https://ncbi.nlm.nih.gov/pmc/articles/PMC5779865/ https://ncbi.nlm.nih.gov/pubmed/29371750 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1051/0004-6361/201629109 |
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