Physics
Scientific paper
Jan 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996plas.work..125f&link_type=abstract
Proceedings of the Fourth Brazilian Meeting on Plasma Physics and the Sixth Brazilian Plasma Astrophysics Workshop, p. 125
Physics
Type 3 Bursts, Solar Radio Bursts, Plasmas (Physics), Plasma Radiation, Emission Spectra, Damping, Spectrometers, Sensitivity, High Resolution, Electron Beams, Beam Interactions, Chromosphere
Scientific paper
About 350 groups of solar bursts were observed by the high sensitivity, high resolution digital radio decimetric spectroscope (DDHRS), operating in conjunction with a 9-m diameter antenna in decimetric range (1600 plus or minus 100 MHz). Here we report the preliminary analysis of the solar bursts observed in the decimeter band and the observed characteristics, such as time scales and drift rates, which suggest that they are type 3 like bursts and are generated by plasma emission at second harmonic, due the electron beam interaction with chromospheric plasma. Assuming plasma emission as a mechanism of the generation and collisional damping process for decay of these decimetric type 3 bursts, the parameters of the beam responsible for the observed emissions, such as the density and total number of the electrons, have been determined.
Fernandes Francisco Carlos Rocha
Sawant Hanumant S.
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