Physics
Scientific paper
May 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010eguga..12.5954k&link_type=abstract
EGU General Assembly 2010, held 2-7 May, 2010 in Vienna, Austria, p.5954
Physics
Scientific paper
How solar flares accelerate electrons up to relativistic energies is one of the main unsolved problems in Heliophysics. Remote sensing at radio and hard X-ray wavelengths provide crucial diagnostics of flare-accelerated electrons in the solar corona. In-situ observations in interplanetary space give direct observations of flare-accelerated electrons escaping the Sun. In this review, recent results combining these observations are discussed, with a special emphases on future observations with Solar Orbiter and Solar Probe +.
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