By Topic

Modeling of Solar Flare Plasma and Its Radiation

Sign In

Cookies must be enabled to login.After enabling cookies , please use refresh or reload or ctrl+f5 on the browser for the login options.

Formats Non-Member Member
$31 $13
Learn how you can qualify for the best price for this item!
Become an IEEE Member or Subscribe to
IEEE Xplore for exclusive pricing!
close button

puzzle piece

IEEE membership options for an individual and IEEE Xplore subscriptions for an organization offer the most affordable access to essential journal articles, conference papers, standards, eBooks, and eLearning courses.

Learn more about:

IEEE membership

IEEE Xplore subscriptions

5 Author(s)
Varady, M. ; Prirodovedecka Fakulta, Univerzity J. E. Purkyne, Ústí nad Labem, Czech Republic ; Kašparová, J. ; Moravec, Z. ; Heinzel, P.
more authors

We present a modular and highly versatile test particle-radiative hydrodynamic code which simultaneously models the particle beam energy transport and deposition, the corresponding explosive response of the flare atmosphere and the NLTE (NLTE, plasma and radiation out of the local thermodynamic equilibrium) radiative transfer for partly ionized hydrogen in the chromosphere and photosphere. The computational domain covers the photosphere, the chromosphere, the transition region, and the corona with the initial hydrostatic preflare atmosphere. To demonstrate the potential of the code, we calculate the time evolution of the Balmer line profiles corresponding to the time variation of the electron beam flux derived from the observed flare hard X-ray emission.

Published in:

Plasma Science, IEEE Transactions on  (Volume:38 ,  Issue: 9 )