Radio observations of total solar eclipse of November 3, 1994 at Chapeco (Brzil)

被引：0

作者：

Sawant, H.S. ^{[1
]}

Srivastava, N. ^{[1
]}

Trigoso, H.E. ^{[1
]}

Sobral, J.H.A. ^{[1
]}

Fernandes, F.C.R. ^{[1
]}

Cecatto, J.R. ^{[1
]}

Subramanian, K.R. ^{[1
]}

机构：

[1] Divisão de Astrofísica, INPE, C. P. 515, Sao Jose dos Campos - SP, 12201-970, Brazil

来源：

Advances in Space Research | / 20卷 / 12期

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摘要：

Radio observations of the eclipse on November 3, 1994, were carried out at Chapeco, 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 ( [similar to] 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 [similar to] 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. © 1997 COSPAR. Published by Elsevier Science Ltd.

引用

页码：2359 / 2363

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