Evidence for two different physical mechanisms for acceleration of solar energetic particles (SEPs) arose 50 years ago with radio observations of type III bursts, produced by outward streaming electrons, and type II bursts from coronal and interplanetary shock waves. Since that time we have found that the former are related to “impulsive” SEP events from impulsive flares or jets. Here, resonant stochastic acceleration, related to magnetic reconnection involving open field lines, produces not only electrons but 1000-fold enhancements of
Beschreibung
The Two Sources of Solar Energetic Particles - Online First - Springer
%0 Journal Article
%1 reames2013
%A Reames, Donald V.
%D 2013
%I Springer Netherlands
%J Space Science Reviews
%K energetic particles solar
%P 1-40
%R 10.1007/s11214-013-9958-9
%T The Two Sources of Solar Energetic Particles
%U http://dx.doi.org/10.1007/s11214-013-9958-9
%X Evidence for two different physical mechanisms for acceleration of solar energetic particles (SEPs) arose 50 years ago with radio observations of type III bursts, produced by outward streaming electrons, and type II bursts from coronal and interplanetary shock waves. Since that time we have found that the former are related to “impulsive” SEP events from impulsive flares or jets. Here, resonant stochastic acceleration, related to magnetic reconnection involving open field lines, produces not only electrons but 1000-fold enhancements of
@article{reames2013,
abstract = {Evidence for two different physical mechanisms for acceleration of solar energetic particles (SEPs) arose 50 years ago with radio observations of type III bursts, produced by outward streaming electrons, and type II bursts from coronal and interplanetary shock waves. Since that time we have found that the former are related to “impulsive” SEP events from impulsive flares or jets. Here, resonant stochastic acceleration, related to magnetic reconnection involving open field lines, produces not only electrons but 1000-fold enhancements of },
added-at = {2013-02-28T10:30:10.000+0100},
author = {Reames, Donald V.},
biburl = {https://www.bibsonomy.org/bibtex/2fcbd362cf5d736defb8a42156d349273/ursg},
description = {The Two Sources of Solar Energetic Particles - Online First - Springer},
doi = {10.1007/s11214-013-9958-9},
interhash = {cd3a402a78ff8e543d6b4f97e677af0d},
intrahash = {fcbd362cf5d736defb8a42156d349273},
issn = {0038-6308},
journal = {Space Science Reviews},
keywords = {energetic particles solar},
language = {English},
pages = {1-40},
publisher = {Springer Netherlands},
timestamp = {2013-02-28T10:30:10.000+0100},
title = {The Two Sources of Solar Energetic Particles},
url = {http://dx.doi.org/10.1007/s11214-013-9958-9},
year = 2013
}