Submillimeter/IR solar bursts from high energy electrons

Details Submillimeter/IR solar bursts from high energy electrons Submillimeter/IR solar bursts from high energy electrons

Jun 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..374..379k&link_type=abstract

High energy solar physics. AIP Conference Proceedings, Volume 374, pp. 379-392 (1996).

Physics

3

Solar Electromagnetic Emission

Scientific paper

There are various observational results which suggest that certain solar bursts have spectral components extending into the submm-w and infrared range. This is essentially unexplored for burst emissions in the continuum. The short time scales of burst structures (tens of milliseconds) correlated to hard X-rays bring serious constraints for interpretation. One possibility is to assume the impulsive phase made of explosions of compact synchrotron sources and self inverse-Compton reducing the electrons energy, producing the correlated spiky hard X-ray component. A new project for a solar submm-w telescope is now being developed in a collaboration between groups in Brazil, Switzerland and Argentina. It is expected to bring important observational clues for the understanding of the initial phase of flares.

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