Detection of durable non-thermal processes in quiescent solar active regions

Details Detection of durable non-thermal processes in quiescent solar active regions Detection of durable non-thermal processes in quiescent solar active regions

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001a%26at...20..459b&link_type=abstract

Astronomical and Astrophysical Transactions, vol. 20, Issue 3, pp.459-465

Astronomy and Astrophysics

Astronomy

3

Microburst, Polarization, Spectrum

Scientific paper

The problem of energy release over a wide dynamic range is key to understanding coronal heating. The detection of the smallest discrete release of energy is important for confirming the modern existing theories. Such processes are recorded on the radio telescope RATAN-600 during weak active region observations at several microwave wavelengths. The flux sensitivity of the radio telescope RATAN-600 in one-dimensional scans is about (5-10) Jy at several-decimeter wavelengths. This allowed us to discover two new types the sources in the active region: a continuum source and microbursts (MB). Here we describe the main parameters of the sources and possible interpretations of the emission.

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