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Initial solar observations with Prototype Brazilian Decimetric Array

Published online by Cambridge University Press:  01 November 2006

F.C.R. Fernandes ,
R. Ramesh ,
J.R. Cecatto ,
C. Faria ,
M.C. Andrade ,
K.R. Subramanian ,
M.S. Sundara Rajan  and
H.S. Sawant
F.C.R. Fernandes
Affiliation:
INPE - National Institute for Space Research, São José dos Campos, SP, Brazil email: [email protected]. Present address: INPE / DAS, C.P. 515 12201-970 São José dos Campos, SP, Brazil.
R. Ramesh
Affiliation:
Indian Instute of Astrophyiscs, Bangalore, India email: [email protected]
J.R. Cecatto
Affiliation:
INPE - National Institute for Space Research, São José dos Campos, SP, Brazil email: [email protected].
C. Faria
Affiliation:
INPE - National Institute for Space Research, São José dos Campos, SP, Brazil email: [email protected]. Computer Department, Catholic University of Minas Gerais, Poços de Caldas, MG, Brazil email: [email protected]
M.C. Andrade
Affiliation:
INPE - National Institute for Space Research, São José dos Campos, SP, Brazil email: [email protected].
K.R. Subramanian
Affiliation:
Indian Instute of Astrophyiscs, Bangalore, India email: [email protected]
M.S. Sundara Rajan
Affiliation:
Indian Instute of Astrophyiscs, Bangalore, India email: [email protected]
H.S. Sawant
Affiliation:
INPE - National Institute for Space Research, São José dos Campos, SP, Brazil email: [email protected].
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Abstract

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The Prototype Brazilian Decimetre Array (PBDA) consists of 5 element alt-azimuth mounted parabolic dishes of 4-m diameter, having baselines up to 216 m in East-West direction. We present initial solar observations carried out with the PBDA during the period 22$^{\hbox{\scriptsize{nd}}}$ November to 11$^{\hbox{\scriptsize{th}}}$ December, 2004. The frequency of observation was 1.6 GHz. The temporal and spatial resolution were 100 ms and 3 arcmin, respectively.

Keywords

Interferometrysolar observations
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S233: Solar Activity and its Magnetic Origin , March 2006 , pp. 445 - 446
Copyright
© 2006 International Astronomical Union