%0 Journal Article
%@holdercode {isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S}
%@nexthigherunit 8JMKD3MGPCW/3ETR8EH
%3 1-s2.0-S0273117797010478-main.pdf
%X Radio observations of the eclipse on November 3, 1994, were carried out at Chapecó, 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.
%N 12
%T Radio observations of total solar eclipse of November 3, 1994 at Chapecó (Brazil)
%@secondarytype PRE PI
%@archivingpolicy denypublisher denyfinaldraft24
%@usergroup administrator
%@usergroup marciana
%@group DAS-INPE-MCT-BR
%@group
%@group
%@group DAS-INPE-MCT-BR
%@group
%@group DAS-INPE-MCT-BR
%@copyholder SID/SCD
%@secondarykey INPE-10291-TDI/910
%@issn 0273-1177
%2 sid.inpe.br/marciana/2004/01.22.14.21.20
%B Advances in Space Research
%@versiontype publisher
%P 2359-2363
%4 sid.inpe.br/marciana/2004/01.22.14.21
%@documentstage not transferred
%D 1997
%V 20
%@doi 10.1016/S0273-1177(97)01047-8;
%A Sawant, Hanumant Shankar,
%A Srivastava, N.,
%A Trigoso, H. E.,
%A Sobral, José Humberto Andrade,
%A Fernandes, Francisco Carlos Rocha,
%A Cecatto, José Roberto,
%A Subramanian, K. R.,
%@dissemination WEBSCI; PORTALCAPES; MGA; COMPENDEX.
%@area CEA