Two-dimensional distributions of physical parameters in the prominence of 1984 March 23

Details Two-dimensional distributions of physical parameters in the prominence of 1984 March 23 Two-dimensional distributions of physical parameters in the prominence of 1984 March 23

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987cha%26a..11..215z&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 11, Issue 3, p. 215-220.

Astronomy and Astrophysics

Astrophysics

2

The Sun

Scientific paper

The spectral lines Hα Hβ and CaII K of a quiescent prominence are studied using the completely linearized model. The physical parameters (Te, vt, NH) at several locations are obtained. Itis shown: (1) Near the axis of the prominence, kinetic temperature and hydrogen density decrease, while microturbulent velocity increases, with increasing height. (2) Near the edge, the kinetic temperature does not vary with height; but it increases from the center to the edge. (3) Hydrostatic equilibrium does not hold in prominences, and magnetic field plays an important role in supporting them.

Affiliated with

Also associated with

No associations

Rating

Two-dimensional distributions of physical parameters in the prominence of 1984 March 23 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 Two-dimensional distributions of physical parameters in the prominence of 1984 March 23, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Two-dimensional distributions of physical parameters in the prominence of 1984 March 23 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1673017