Dynamics and Energetics of Stellar Flares

Details Dynamics and Energetics of Stellar Flares Dynamics and Energetics of Stellar Flares

Jul 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999hst..prop.8040l&link_type=abstract

HST Proposal ID #8040

Physics

Hst Proposal Id #8040 Cool Stars

Scientific paper

Mode 1.3 echelle spectra will be used to explore the dynamics and energetics of flares on M dwarfs. We will use line fluxes to determine emission measure distributions {10^4 to 10^7 K} and electron densities as a function of time during the flare. Line shapes and Doppler shifts will be used to characterize plasma dynamics {flows, turbulence} throughout the flare. We will search for cooling via UV continuum emission in the early phases of the flare. Nonflare spectra will be used to model the quiescent atmosphere.

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