Physical Parameters of a Flare Derived from Multi-line 2D Spectroscopy

Details Physical Parameters of a Flare Derived from Multi-line 2D Spectroscopy Physical Parameters of a Flare Derived from Multi-line 2D Spectroscopy

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001chjaa...1..460l&link_type=abstract

Chinese Journal of Astronomy & Astrophysics

Astronomy and Astrophysics

Astrophysics

Sun: Flares, Sun: Chromosphere

Scientific paper

Time series of 2D spectra of Hα and Ca II λ 8542 for a flare of 1999 December 22 are obtained and analyzed with a new fitting technique. The method we proposed can simultaneously yield the four parameters: the line source function, the optical thickness at line center, the line-of-sight velocity and the Doppler width. We present the spatial distributions of the physical parameters and their temporal evolutions determined from the 2D spectra. Our results are consistent with the general picture predicted by the flare dynamic models.

Affiliated with

Also associated with

No associations

Rating

Physical Parameters of a Flare Derived from Multi-line 2D Spectroscopy 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 Physical Parameters of a Flare Derived from Multi-line 2D Spectroscopy, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Physical Parameters of a Flare Derived from Multi-line 2D Spectroscopy will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1104762