2D MHD AND 1D HD MODELS OF A SOLAR FLARE—A COMPREHENSIVE COMPARISON OF THE RESULTS
- 29 October 2015
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 813 (1) , 70
Abstract
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This publication has 49 references indexed in Scilit:
- Models of the Solar Chromosphere and Transition Region from SUMER and HRTS Observations: Formation of the Extreme‐Ultraviolet Spectrum of Hydrogen, Carbon, and OxygenThe Astrophysical Journal Supplement Series, 2008
- A Statistical Model of the Inhomogeneous Corona Constrained by Triple‐Filter Measurements of Elementary Loop Strands withTRACEThe Astrophysical Journal, 2007
- What Do We (Not) Know Theoretically about Solar Neutrino Fluxes?Physical Review Letters, 2004
- Flare Plasma Cooling from 30 MK down to 1 MK modeled from Yohkoh, GOES, and TRACE observations during the Bastille Day Event (14 July 2000)Solar Physics, 2001
- Deconvolution of Directly Precipitating and Trap‐precipitating Electrons in Solar Flare Hard X‐Rays. III.YohkohHard X‐Ray Telescope Data AnalysisThe Astrophysical Journal, 1999
- EIT: Extreme-ultraviolet Imaging Telescope for the SOHO missionSolar Physics, 1995
- Cooling of solar flares plasmas. 1: Theoretical considerationsThe Astrophysical Journal, 1995
- Some implications of the nanoflare conceptThe Astrophysical Journal, 1994
- The energetics of chromospheric evaporation in solar flaresThe Astrophysical Journal, 1984
- The deduction of energy spectra of non-thermal electrons in flares from the observed dynamic spectra of hard X-ray burstsSolar Physics, 1971