On the Relation between Flares and CMEs

Details On the Relation between Flares and CMEs On the Relation between Flares and CMEs

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002mwoc.conf..309n&link_type=abstract

Multi-Wavelength Observations of Coronal Structure and Dynamics -- Yohkoh 10th Anniversary Meeting. Proceedings of the conferenc

Physics

1

Scientific paper

On the relation between flares and CMEs N. V. Nitta, H. S. Hudson As we reported elsewhere (GRL, in press), six recurrent `halo' coronal mass ejections (CMEs) occurred (in November 2000) during a 60-hour period in clear association with major flares in an active region on the solar disk. The region was undergoing dynamic restructuring due to flux emergence. The flares were not long-decay events (LDEs) in terms of soft X-ray light curves and morphologies, although, in the impulsive phase, they produced ejections in soft X-rays that are characteristic of CMEs. In this presentation, we extend our study to more flare/CME events, including analysis of some data taken at and near Earth. We address (but will not fully answer) questions including (1) Are flare-associated CMEs triggered differently from those without flare association, (2) Can we isolate observational signatures that are more relevant to flares or CMEs, (3) What is the relevance of solar coronal phenomena to solar energetic particles and geomagnetic indices.

Affiliated with

Also associated with

No associations

Rating

On the Relation between Flares and CMEs 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 Relation between Flares and CMEs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the Relation between Flares and CMEs will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1838596