Phenomenology of coronal mass ejections

Details Phenomenology of coronal mass ejections Phenomenology of coronal mass ejections

Apr 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999arep...43..255m&link_type=abstract

Astronomy Reports, Volume 43, Issue 4, April 1999, pp.255-266

Astronomy and Astrophysics

Astronomy

Scientific paper

An attempt to describe the phenomenology of solar coronal mass ejections (CMEs) at all wavelength bands is undertaken. The development of several typical CMEs in 1996 and 1997 is considered in detail. Among the properties revealed, we especially emphasize (1) the presence of initial eruption prominences that are relatively distant from each other, (2) the development of CMEs from two eruption sites, and (3) the connection of CMEs with structural evolution, i.e., large-scale solar-activity complexes. In addition to determining the basic properties of CMEs, we compare scenarios for CMEs and flares and search for common features in the natures of these phenomena, which have very different temporal and spatial scales. A qualitative model for the above phenomena is put forward.

Affiliated with

Also associated with

No associations

Rating

Phenomenology of 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 Phenomenology of coronal mass ejections, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Phenomenology of coronal mass ejections will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1429935