HR: 1340h
AN: SH33B-0377    [Abstracts]
TI: Coronal Radio Observations of Inferred Solar Near-Relativistic Electron Injections
AU: * Kahler, S
EM: Stephen.Kahler@hanscom.af.mil
AF: Air Force Research Laboratory, AFRL/VSBXS 29 Randolph Rd, Hanscom AFB, MA 01731 United States
AU: Aurass, H
EM: haurass@aip.de
AF: Astrophysikalisches Institut Potsdam, An der Sternwarte 16, Potsdam, D-14482 Germany
AU: Mann, G
EM: gmann@aip.de
AF: Astrophysikalisches Institut Potsdam, An der Sternwarte 16, Potsdam, D-14482 Germany
AU: Klassen, A
EM: klassen@physik.uni-kiel.de
AF: Institut fur Experimentelle und Angewandte Physik, University of Kiel Leibnizstrasse 11, Kiel, D-24118 Germany
AB: The solar injections of near-relativistic electrons observed at 1 AU appear to be systematically delayed by ~ 10 min from the associated flare impulsive phases. We select for detailed study 80 electron events well observed by the 3DP particle detector on the WIND spacecraft during times of 40 -1600 MHz solar observations by the AIP radio telescope in Tremsdorf, Germany. The calculated solar injection times are compared with the coronal radio emissions to search for characteristic signatures of electron acceleration/injection. We find no single radio signature characteristic of the electron injection process. The results are compared with scenarios for the delayed injections suggested by other investigators.
DE: 7514 Energetic particles (2114)
DE: 7519 Flares
DE: 7534 Radio emissions
SC: SPA-Solar and Heliospheric Physics [SH]
MN: Fall Meeting 2005