Wavelet Decomposition of Submillimeter Solar Radio Bursts

Details Wavelet Decomposition of Submillimeter Solar Radio Bursts Wavelet Decomposition of Submillimeter Solar Radio Bursts

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003soph..218..211m&link_type=abstract

Solar Physics, v. 218, Issue 1, p. 211-220 (2003).

Physics

3

Scientific paper

We present the results of wavelet decomposition of fast-time structures during four solar flares observed by the Solar Submillimeter-wave Telescope at 212 GHz. The result of the analysis shows (1) observational evidence on the existence of submm-emission time variations in the range from a few tens of millisecond up to few seconds during solar flares, and (2) that when a solar flare is in progress the time scales reduce as the bulk of the emission flux time variations is increasing.

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