Number of the records: 1
Solar flares: observation vs simulations
- 1.
SYSNO ASEP 0360906 Document Type C - Proceedings Paper (int. conf.) R&D Document Type Conference Paper Title Solar flares: observation vs simulations Author(s) Rubio da Costa, F. (IT)
Zuccarello, F. (IT)
Labrosse, N. (GB)
Fletcher, L. (GB)
Prosecký, Tomáš (ASU-R)
Kašparová, Jana (ASU-R) RID, ORCIDNumber of authors 6 Source Title Advances in Plasma Astrophysics. - Cambridge : Cambridge University Press, 2011 / Bonanno A. - ISSN 1743-9213 - ISBN 9780521197410 Pages s. 182-184 Number of pages 3 s. Action Symposium of the International Astronomical Union /274./ Event date 06.09.2010-10.09.2010 VEvent location Giardini Naxos Country IT - Italy Event type WRD Language eng - English Country GB - United Kingdom Keywords numerical methods ; radiative transfer ; solar flares Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics CEZ AV0Z10030501 - ASU-R (2005-2011) UT WOS 000305161800040 DOI 10.1017/S1743921311006880 Annotation In order to study the properties of faint, moderate and bright flares, we simulate the conditions of the solar atmosphere using a radiative hydrodynamic model (Abbett & Hawley, 1999). A constant beam of non-thermal electrons is injected at the apex of a 1D coronal loop and heating from thermal soft X-ray emission is included. We compare the results with some observational data in Ly-α (using TRACE 1216 and 1600 ˚A data and estimating the “pure” Ly-α emission) and in Hα (data taken with a Multichannel Flare Spectrograph, at the Ondrejov Observatory). Workplace Astronomical Institute Contact Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2012
Number of the records: 1