Understanding solar flares from opticalobservations: How do particle beams affect the lower atmosphere?
Author:
Publisher
Elsevier BV
Subject
Space and Planetary Science,Aerospace Engineering,General Earth and Planetary Sciences,Atmospheric Science,Geophysics,Astronomy and Astrophysics
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5. Non-LTE radiative hydrodynamic interactions in the solar chromosphere;Carlsson,1990
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1. Connection between the appearance of γ-ray sources and Hα line impact linear polarization in the July 23, 2002 flare;Astronomy Letters;2015-10
2. Solar chromosphere flare spectrograph;Solar Physics and Space Weather Instrumentation V;2013-09-26
3. Sizes of flaring kernels in various parts of the Hα line profile;Annales Geophysicae;2008-10-15
4. Non-thermal particle effects on the Hα and Hβ line profiles in the 18 August 2002 solar flare;Annales Geophysicae;2008-10-15
5. The multi-wavelength study of the effect of energetic particle beams on the chromospheric emission in the 25th July 2004 solar flare;Advances in Space Research;2007-01
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