http://www.cnr.it/ontology/cnr/individuo/prodotto/ID204467
EMPIRICAL DETERMINATION OF THE ENERGY LOSS RATE OF ACCELERATED ELECTRONS IN A WELL-OBSERVED SOLAR FLARE (Articolo in rivista)
- Type
- Label
- EMPIRICAL DETERMINATION OF THE ENERGY LOSS RATE OF ACCELERATED ELECTRONS IN A WELL-OBSERVED SOLAR FLARE (Articolo in rivista) (literal)
- Anno
- 2012-01-01T00:00:00+01:00 (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#doi
- 10.1088/0004-637X/751/2/129 (literal)
- Alternative label
Gabriele Torre1, Nicola Pinamonti1, A. Gordon Emslie2, Jingnan Guo1, Anna Maria Massone3, and Michele Piana1,3 (2012)
EMPIRICAL DETERMINATION OF THE ENERGY LOSS RATE OF ACCELERATED ELECTRONS IN A WELL-OBSERVED SOLAR FLARE
in The Astrophysical journal
(literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
- Gabriele Torre1, Nicola Pinamonti1, A. Gordon Emslie2, Jingnan Guo1, Anna Maria Massone3, and Michele Piana1,3 (literal)
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- Rivista
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- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroFascicolo
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
- 1 Dipartimento di Matematica, Università di Genova, Genova, via Dodecaneso 35, 16146 Genova, Italy
2 Department of Physics and Astronomy, Western Kentucky University, Bowling Green, KY 42101, USA
3 CNR-SPIN, Via Dodecaneso 33, I-16146 Genova, Italy (literal)
- Titolo
- EMPIRICAL DETERMINATION OF THE ENERGY LOSS RATE OF ACCELERATED ELECTRONS IN A WELL-OBSERVED SOLAR FLARE (literal)
- Abstract
- We present electron images of an extended solar flare source, deduced from RHESSI hard X-ray imaging spectroscopy data. We apply the electron continuity equation to these maps in order to determine empirically the form of the energy loss rate for the bremsstrahlung-emitting electrons. We show that this form is consistent with an energy transport model involving Coulomb collisions in a target with a temperature of about 2 x 107 K, with a continuous injection of fresh deka-keV electrons at a rate of approximately 10-2 electrons s-1 per ambient electron. (literal)
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