Physics
Scientific paper
Sep 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008espm...122.105m&link_type=abstract
"12th European Solar Physics Meeting, Freiburg, Germany, held September, 8-12, 2008. Online at http://espm.kis.uni-freiburg.de/,
Physics
Scientific paper
The 22 minutes lasting interval of broadband dm-radio pulsations observed simultaneously during a decay phase of the June 6, 2000 flare by the Brazilian Solar Spectroscope (BSS) and Ondrejov radiospectrograph in frequency range 1200-4500 MHz has been analyzed. We have realized that dominant periods (32-64 s) belong to fast wave trains with a tadpole pattern in their wavelet power spectra. The whole time interval contains series of about 4 wave trains. These trains propagate in whole frequency range 1200-4500 MHz. The propagation of individual trains at lower levels of the solar atmosphere (higher frequencies) is different from propagation of individual trains at higher ones (lower frequencies). The wave trains at the same frequencies but in different time subintervals have some common as well as different properties. The main statistical parameters (periodical, quasi-periodical and decay phase) of these wave trains in their wavelet power spectra have been studied and the first results will be presented and discussed.
Andrade M. C.
Cecatto José R.
Fernandes Francisco Carlos Rocha
Jiřička Karel
Karlicky Marian
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