2D radiative modelling of He I spectral lines formed in solar prominences

Details 2D radiative modelling of He I spectral lines formed in solar prominences 2D radiative modelling of He I spectral lines formed in solar prominences

2007-12-11

arxiv.org/abs/0712.1701v2

Astronomy and Astrophysics

Astrophysics

4 pages, 2 figures (to appear in the Procs. of Solar Polarization Workshop #5, eds. Berdyugina, Nagendra and Ramelli), revised

Scientific paper

We present preliminary results of 2D radiative modelling of He I lines in solar prominences, using a new numerical code developed by us (Leger, Chevallier and Paletou 2007). It treats self-consistently the radiation transfer and the non-LTE statistical equilibrium of H and, in a second stage, the one of He using a detailed atomic model. Preliminary comparisons with new visible plus near-infrared observations made at high spectral resolution with THeMIS are very satisfactory.

Affiliated with

Also associated with

No associations

Rating

2D radiative modelling of He I spectral lines formed in 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 2D radiative modelling of He I spectral lines formed in solar prominences, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and 2D radiative modelling of He I spectral lines formed in solar prominences will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-474335