Magnetic structure of solar prominences

Details Magnetic structure of solar prominences Magnetic structure of solar prominences

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992angeo..10..344v&link_type=abstract

Annales Geophysicae (ISSN 0992-7689), vol. 10, no. 6, June 1992, p. 344-353.

Physics

10

Solar Corona, Solar Magnetic Field, Solar Prominences, Magnetohydrodynamic Stability, Stellar Mass Ejection, Stellar Models

Scientific paper

The most important observational aspects and physical interpretations related to the solar prominence phenomenon are summarized. General properties, evolution, internal structure, the process of eruption, and the relation to coronal mass ejections and the associated electric current system are included. A schematic drawing of a prominence and its environment is given.

Affiliated with

Also associated with

No associations

Rating

Magnetic structure of solar prominences 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 Magnetic structure of solar prominences, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Magnetic structure of solar prominences will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1199480