Reconnection-Driven Coronal-Hole Jets with Gravity and Solar Wind
Reconnection-Driven Coronal-Hole Jets with Gravity and Solar Wind
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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Coronal-hole jets occur ubiquitously in solar coronal holes, at EUV and X-ray bright points associated with intrusions of minority magnetic polarity. The embedded-bipole model for these jets posits that they are driven by explosive, fast reconnection between the stressed closed field of the embedded bipole and the open field of the surrounding coro...
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Reconnection-Driven Coronal-Hole Jets with Gravity and Solar Wind
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TN_cdi_proquest_journals_2074987859
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2074987859
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1606.09201
