Plasma Motion in Crossed Fields and Halo-Type Coronal Mass Ejections

Details Plasma Motion in Crossed Fields and Halo-Type Coronal Mass Ejections Plasma Motion in Crossed Fields and Halo-Type Coronal Mass Ejections

Jul 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002arep...46..591m&link_type=abstract

Astronomy Reports, Vol. 46, Issue 7, pp. 591-596

Astronomy and Astrophysics

Astronomy

Scientific paper

Halo-type motions of plasma in the solar corona—so-called coronal mass ejections (CME)—are considered. This type of CME is relatively rare due to the requirement for a particular orientation of the magnetic-moment vector M (parallel to the line of sight). Variations in |M| may be due to the rapid motion of filaments with a characteristic time scale ≅103 s. The drifts in the crossed fields have speeds of ≅200 1000 km/s and can account for the basic features of the CME geometry.

Affiliated with

Also associated with

No associations

Rating

Plasma Motion in Crossed Fields and Halo-Type 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 Plasma Motion in Crossed Fields and Halo-Type Coronal Mass Ejections, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Plasma Motion in Crossed Fields and Halo-Type Coronal Mass Ejections will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-961050