Coronal Mass Ejections from Magnetic Systems Encompassing Filament Channels Without Filaments

Details Coronal Mass Ejections from Magnetic Systems Encompassing Filament Channels Without Filaments Coronal Mass Ejections from Magnetic Systems Encompassing Filament Channels Without Filaments

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012soph..277..185p&link_type=abstract

Solar Physics, Volume 277, Issue 1, pp.185-201

Physics

Coronal Mass Ejections, Low Coronal Signatures, Initiation And Propagation, Magnetic Fields, Corona, Prominences, Formation And Evolution, Filaments, Filament Mass

Scientific paper

Well-developed filament channels may be present in the solar atmosphere even when there is no trace of filament material inside them. Such magnetic systems with filament channels without filaments can result in coronal mass ejections that might appear to have no corresponding solar surface source regions. In this case study, we analyze CMEs on 9 August 2001 and 3 March 2011 and trace their origins to magnetic systems with filament channels containing no obvious filament material on the days around the eruptions.

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