Stellar Flares, Superflares, and Coronal Mass Ejections—Entering the Big Data Era
Stellar Flares, Superflares, and Coronal Mass Ejections—Entering the Big Data Era
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Publisher
Basel: MDPI AG
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Language
English
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Publisher
Basel: MDPI AG
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Contents
Flares, sometimes accompanied by coronal mass ejections (CMEs), are the result of sudden changes in the magnetic field of stars with high energy release through magnetic reconnection, which can be observed across a wide range of the electromagnetic spectrum from radio waves to the optical range to X-rays. In our observational review, we attempt to...
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Full title
Stellar Flares, Superflares, and Coronal Mass Ejections—Entering the Big Data Era
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TN_cdi_doaj_primary_oai_doaj_org_article_243f83c1fa4e4ce8a8d9cf2a91e663d8
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_doaj_primary_oai_doaj_org_article_243f83c1fa4e4ce8a8d9cf2a91e663d8
Other Identifiers
ISSN
2218-1997
E-ISSN
2218-1997
DOI
10.3390/universe10080313
