@Article{SawantCecDenGarHur:1993:HiSpRe,
author = "Sawant, Hanumant Shankar and Cecatto, Jose Roberto and Dennis, B.
R. and Gary, D. E. and Hurford, G. J",
title = "High spectral resolution, high sensitivity microwave and
associated hard x-ray bursts",
journal = "Advances in Space Research",
year = "1993",
volume = "13",
number = "9",
pages = "(9)191--(9)194",
keywords = "ASTROFISICA.",
abstract = "We have carried out mm-wavelength (18 - 23) GHz observations of
solar bursts in June 1989, in Brazil. Nine of the bursts were
observed simultaneously with the Hard X-ray Burst Spectrometer
(HXRBS) on the Solar Maximimum Mission (SMM). The Owens Valley
Radio Observatory (OVRO) observed five of these events from 1 to
18 GHz. To date, we have analyzed six of these events and the
preliminary results are: (i) The turnover frequency of all of
these bursts were in the frequency range of 7 - 11 GHz and the
radio spectral index ranged from -0.3 to -5.3; (ii) In three
bursts, dominant features of high energy (>-200 keV) X-rays
coincided in time with mm-wavelenght peaks, suggesting that the
high energy electrons are responsible for the mm-wavelenght
emission.",
issn = "0273-1177",
label = "7166",
language = "en",
urlaccessdate = "28 abr. 2024"
}