On the two classes of filament-prominence disappearance and their relation to coronal mass ejections

Details On the two classes of filament-prominence disappearance and their relation to coronal mass ejections On the two classes of filament-prominence disappearance and their relation to coronal mass ejections

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995soph..158..269m&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 158, no. 2, p. 269-281

Physics

23

Solar Corona, Solar Physics, Solar Prominences, Stellar Mass Ejection, Sun, Dynamic Stability, Solar Limb, Thermal Stability

Scientific paper

We analyze the phenomenon of sudden disappearance (DB) of quiescent filaments and prominences, with examples of the two classes (dynamic and thermal DB) observed on the solar disk and at the limb. The differences between their dynamics are discussed, and it is shown that only dynamic DBs are associated with coronal mass ejections (CME), whereas thermal DBs are only local disturbances of the lower corona. We finish with a discussion of DBs detected on the disk and limb, to explain the statistical differences between disappearance of filaments and the production of CME.

Affiliated with

Also associated with

No associations

Rating

On the two classes of filament-prominence disappearance and their relation to coronal mass ejections does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with On the two classes of filament-prominence disappearance and their relation to coronal mass ejections, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the two classes of filament-prominence disappearance and their relation to coronal mass ejections will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1549848