@Article{SawantSrTrSoFeCeSu:1997:RaObTo,
author = "Sawant, Hanumant Shankar and Srivastava, N. and Trigoso, H. E. and
Sobral, Jos{\'e} Humberto Andrade and Fernandes, Francisco Carlos
Rocha and Cecatto, Jos{\'e} Roberto and Subramanian, K. R.",
title = "Radio observations of total solar eclipse of November 3, 1994 at
Chapec{\'o} (Brazil)",
journal = "Advances in Space Research",
year = "1997",
volume = "20",
number = "12",
pages = "2359--2363",
abstract = "Radio observations of the eclipse on November 3, 1994, were
carried out at Chapec{\'o}, Brazil by using a decimetric
spectrograph having high spectral and time resolution. The light
curve shows that: (1) Time variation of the radio flux before the
totality was more compared to that after. (2) During the totality
radio emission at 1.5 GHz was observed. Advantage of high spatial
resolution (~ 3.2 arc sec) possible during solar eclipse enabled
us to determine the height of radio emission at 1.5 GHz. (3)
Microwave bursts were observed associated with metric Type III-RS
bursts. The source size of one of the microwave bursts was ~ 7 arc
sec and its physical parameters have been estimated. (4) The time
difference between radio and optical contacts suggested for the
first time asymmetrical limb brightening at 1.5 GHz.",
copyholder = "SID/SCD",
doi = "{10.1016/S0273-1177(97)01047-8;}",
url = "http://dx.doi.org/{10.1016/S0273-1177(97)01047-8;}",
issn = "0273-1177",
language = "en",
targetfile = "1-s2.0-S0273117797010478-main.pdf",
urlaccessdate = "09 maio 2024"
}