Chromospheric Response to Non-Thermal Electrons During Flares Using RHESSI and SOHO/CDS

Details Chromospheric Response to Non-Thermal Electrons During Flares Using RHESSI and SOHO/CDS Chromospheric Response to Non-Thermal Electrons During Flares Using RHESSI and SOHO/CDS

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsp52a..04m&link_type=abstract

American Geophysical Union, Spring Meeting 2005, abstract #SP52A-04

Physics

7507 Chromosphere, 7519 Flares, 7546 Transition Region, 7549 Ultraviolet Emissions, 7554 X Rays, Gamma Rays, And Neutrinos

Scientific paper

Many current solar flare models predict a relationship between the amount of energy deposited in the chromospheric and transition region layers of the solar atmosphere by non-thermal electrons, and the velocity at which this superheated material rises. For the first time, we present findings from simultaneous observations of loop footpoints using RHESSI and SOHO/CDS. RHESSI HXR images and spectra are used to determine the flux of non-thermal electrons using the thick-target bremsstrahlung model, while upflow velocities in the Fe XIX emission line are observed using CDS.

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