Lehtinen, N. J., S. Pohjolainen, K. Huttunen-Heikinmaa, R. Vainio, E. Valtonen, and A. E. Hillaris, Sources of SEP Acceleration during a Flare - CME Event, Sol. Phys., 247, 151-169 (2008) (ADS)
(click on the image for a larger version)
Date: 2008 September 10
Update: 2019 November 25
A cartoon based on the event SOL2002-11-09. This paper is a nice example of a multi-wavelength analysis of the persistently obscure relationships between interplanetary particles and flare processes. The cartoon shows how the electron streams from type III bursts can be routed through a shock front, leaving a telltale break in the radio drift rate. Note the multipolar solar magnetic structure and the prior existence of open fields; CME 2 is shown blasting out through a streamer.