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Observations of conduction driven evaporation in the early rise phase of solar flares

ASTRONOMY & ASTROPHYSICS, no. 3 (2009): 891-900

Cited by: 79|Views7

Abstract

Context. The classical flare picture features a beam of electrons, which were accelerated in a site in the corona, hitting the chromosphere. The electrons are stopped in the dense chromospheric plasma, emitting bremsstrahlung in hard X-rays. The ambient material is heated by the deposited energy and expands into the magnetic flare loops, ...More

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