Physics
Scientific paper
Jun 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph...97..345m&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 97, June 1985, p. 345-361.
Physics
11
Centimeter Waves, Solar Flares, Solar Radio Bursts, Brightness Temperature, Magnetic Signatures, Polarization Characteristics, Temporal Distribution, Very Large Array (Vla)
Scientific paper
Using the Very Large Array, solar burst observations have been carried out simultaneously at 6 and 20 cm. Structural changes and preheating have been observed in the flaring regions on time scales of minutes to tens of minutes before the onset of the burst impulsive phase. The 6 cm burst sources are located close to the neutral line, or near the legs of a flaring loop. The 20 cm burst sources show complex and extended structures spatially separated from both the preburst emission and the gradual decay phase of the burst. The authors interpret the observations in terms of a two-component flare model (bulk heating as well as acceleration of particles) and derive the physical parameters of the burst sources.
Kundu Mukul R.
Melozzi Mauro
Shevgaonkar R. K.
No associations
LandOfFree
Simultaneous microwave observations of solar flares at 6 and 20 CM wavelengths using the VLA does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Simultaneous microwave observations of solar flares at 6 and 20 CM wavelengths using the VLA, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Simultaneous microwave observations of solar flares at 6 and 20 CM wavelengths using the VLA will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1670461