%0 Journal Article
%@holdercode {isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S}
%@nexthigherunit 8JMKD3MGPCW/3ETR8EH
%@archivingpolicy denypublisher denyfinaldraft24
%@issn 1364-6826
%@usergroup administrator
%@usergroup jefferson
%3 1.71ST_Sych.pdf
%B Journal of Atmospheric and Solar-Terrestrial Physics
%@dissemination WEBSCI; PORTALCAPES; AGU; MGA; COMPENDEX.
%@secondarykey INPE-11762-PRE/7121
%A Sych, R. A.,
%A Altyntsev, A. T.,
%A Meshalkina, N. S.,
%A Chernov, G. P.,
%A Yihua, Yan,
%T Polarization properties of the microwave subsecond pulses: spatial aspects.
%D 2004
%V x
%N ?
%P 13
%2 sid.inpe.br/marciana/2004/12.06.16.21.20
%4 sid.inpe.br/marciana/2004/12.06.16.21
%K Solar flare, Microwave emission, Spikes, Plasma mechanism of emission, Spike source position, Polarization.
%X The determing the wave mode of subsecond pulses (SSP) is made. It is used data with degree of polarization over 30% and was located at -60 to +60 degrees from the central meridian, where there is no depolarization effect due to the quasi- transverse propagation for the period 2000-2002. Data from the Siberian Solar Radio Telescope (SSRT) with 14 ms time resolution (1D radio scans) and 2-3 min. (2D images); spectra in the range 5.2-7.6 GHz from the radio polarimeters of the National astronomical observatory of China (NAOC), cadence ~5 ms and magnetograms (MDI/SOHO) was used. Our superposition of SSRT radio maps and MDI magnetograms has shown that radio spike sources typically lie near the polarity inversion line of the active region magnetic field. Such an arrangement indicates that spikes are located at the tops of magnetic loops. The ordinary mode of electromagnetic radiation in SSP sources is recorded.
%@language English
%@copyholder SID/SCD
%@e-mailaddress robert@das.inpe.br
%@secondarytype PRE PI
%@area CEA
%@group DAS-INPE-MCT-BR