Diagnostics of the solar atmosphere by inverse methods: hydrogen absorption lines

Details Diagnostics of the solar atmosphere by inverse methods: hydrogen absorption lines Diagnostics of the solar atmosphere by inverse methods: hydrogen absorption lines

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005kfnt...21..461s&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 21, no. 6, p. 461-470

Physics

Scientific paper

We solved non-equilibrium inverse radiation transfer problem in hydrogen lines, that allows one to carry out the diagnostics of the solar photosphere and chromosphere layers. The Tikhonov stabilizers ensure solution stability to noise and input guesses of the reproduced parameters, suppress false oscillations of the solutions. Using hydrogen lines, we performed test diagnostics of the solar photosphere and chromosphere layers: the maximum absolute error of the temperature recovering does not exceed 70 K. When studying non-LTE hydrogen line formation, we used the quantum-mechanical approach to take into account the linear Stark effect.

Affiliated with

Also associated with

No associations

Rating

Diagnostics of the solar atmosphere by inverse methods: hydrogen absorption lines 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 Diagnostics of the solar atmosphere by inverse methods: hydrogen absorption lines, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Diagnostics of the solar atmosphere by inverse methods: hydrogen absorption lines will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1612553