Observations of solar Type II bursts at decameter wavelengths

Details Observations of solar Type II bursts at decameter wavelengths Observations of solar Type II bursts at decameter wavelengths

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003eaeja....14158m&link_type=abstract

EGS - AGU - EUG Joint Assembly, Abstracts from the meeting held in Nice, France, 6 - 11 April 2003, abstract #14158

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The observation results concerning solar Type II bursts, which were obtained with the world largest radio telescope UTR-2 equipped with the new high performance back-end facility, 60-channel spectrometer and digital spectro polarimeter, operating in the frequency band from 10MHz to 30MHz are presented. These bursts are considered to be associated with CME's, which influence essentially on the Solar-Terrestrial relationship. Observed decameter Type II bursts have a fine frequency-time structure, drift slowly (<0.1MHz/s) and sometimes are band-splitting. A typical Type II bursts was observed on July, 7th, 2002, where we note the absence a frequency drift and the presence of a herringbone structure. Some physical characteristics of decameter Type II bursts are discussed.

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