Coronal Mass Ejections and Active Prominences Relationship During Solar Cycle 23

Details Coronal Mass Ejections and Active Prominences Relationship During Solar Cycle 23 Coronal Mass Ejections and Active Prominences Relationship During Solar Cycle 23

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..895..153l&link_type=abstract

FIFTY YEARS OF ROMANIAN ASTROPHYSICS. AIP Conference Proceedings, Volume 895, pp. 153-159 (2007).

Astronomy and Astrophysics

Astrophysics

Coronal Mass Ejection, Prominence Eruptions, Sun Spots, Solar Cycles

Scientific paper

We report the results of a statistical study of the association between active prominences, observed in microwaves by the Nobeyama Radio Heliograph, and coronal mass ejections, observed in white light by LASCO/SOHO. We found that 6.4 % of the observed CMEs are related to active prominences. This low association is due to the differences between the instruments (ground and space based) and the fact that CMEs are related not only to active prominences but also to flares and filaments. On the other hand, we found that only 24.7% of the active prominences are related to CMEs. We suggest that this low association number is due to the poor determination of the CME source region.

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