Radio Diagnostics of the Solar Flare Reconnection

Details Radio Diagnostics of the Solar Flare Reconnection Radio Diagnostics of the Solar Flare Reconnection

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ssrv..121..153k&link_type=abstract

Space Science Reviews, Volume 121, Issue 1-4, pp. 153-164

Computer Science

1

Solar Flare, Magnetic Reconnection, Radio Radiation

Scientific paper

First, high-frequency (HF) slowly drifting pulsating structures are interpreted as radio emissions of electron beams accelerated in the magnetic reconnection volume and injected into magnetic islands (plasmoids). Then, the time evolution of plasma parameters (density, magnetic field, etc.) in a 2-D MHD model of solar flare reconnection is computed numerically. Assuming plasma radio emission from locations where the “double-resonance’’ instability generates upper-hybrid (UH) waves due to unstable distribution function of suprathermal electrons, the radio spectra and spatial source structures in the reconnection region are modeled. By comparison of the modeled and observed spectra a remarkable similarity has been found between the computed narrow-band emission and the observed lace bursts. Finally, a new diagnostics of the reconnection process is proposed.

Affiliated with

Also associated with

No associations

Rating

Radio Diagnostics of the Solar Flare Reconnection does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Radio Diagnostics of the Solar Flare Reconnection, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radio Diagnostics of the Solar Flare Reconnection will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1733349