A spectropolarimetric estimate of energy deposition into the chromosphere during solar flares

Details A spectropolarimetric estimate of energy deposition into the chromosphere during solar flares A spectropolarimetric estimate of energy deposition into the chromosphere during solar flares

May 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999arep...43..340k&link_type=abstract

Astronomy Reports, Volume 43, Issue 5, May 1999, pp.340-343

Astronomy and Astrophysics

Astronomy

Scientific paper

The dependence of the degree of polarization of Hα and Hβ emission in the solar chromosphere during solar flares on the energy of an incident proton beam is calculated assuming that the origin of the observed linear polarization is collisional. Estimates of the lower boundary for the energy of the proton beam are obtained using a model for the kinetics of the propagation of fast protons inside solar-flare magnetic loops together with spectropolarimetric Hα and Hβ observations.

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