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Relationships between sequential chromospheric brightening and the corona
Kirk M.S., Jackiewicz J., , Gilbert H.R.
Published in Cambridge University Press
2016
Volume: 12
   
Pages: 117 - 127
Abstract
The chromosphere is a complex region that acts as an intermediary between the magnetic flux emergence in the photosphere and the magnetic features seen in the corona. Large eruptions in the chromosphere of flares and filaments are often accompanied by ejections of coronal mass off the sun. Several studies have observed fast-moving progressive trains of compact bright points (called Sequential Chromospheric Brightenings or SCBs) streaming away from chromospheric flares that also produce a coronal mass ejection (CME). In this work, we review studies of SCBs and search for commonalties between them. We place these findings into a larger context with contemporary chromospheric and coronal observations. SCBs are fleeting indicators of the solar atmospheric environment as it existed before their associated eruption. Since they appear at the very outset of a flare eruption, SCBs are good early indication of a CME measured in the chromosphere. © International Astronomical Union 2017.
About the journal
JournalData powered by TypesetProceedings of the International Astronomical Union
PublisherData powered by TypesetCambridge University Press
ISSN17439213
Open AccessNo