Dynamics of the Corona Magnetic Field Inferred from Multi-frequency Observations of the 1998 November 5 Solar Flare

Details Dynamics of the Corona Magnetic Field Inferred from Multi-frequency Observations of the 1998 November 5 Solar Flare Dynamics of the Corona Magnetic Field Inferred from Multi-frequency Observations of the 1998 November 5 Solar Flare

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agusm..sp61a11c&link_type=abstract

American Geophysical Union, Spring Meeting 2001, abstract #SP61A-11

Physics

7509 Corona, 7514 Energetic Particles (2114), 7524 Magnetic Fields, 7534 Radio Emissions

Scientific paper

We report multi-frequency observations of a solar Goes M1.5 class flare occurred at about 1335 UT. The event was observed over a wide range of altitudes, between the low corona where ~ 200 keV hard X rays from non-thermal electrons were produced, up to about 0.5 R&sun; , where the electron beams propagated outward. We will discuss these observations in terms of the relation between the production of non-thermal electrons in the low/middle solar atmosphere and the dynamics of the high corona magnetic field traced by spatially resolved dm/metric emitting sources.

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