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Southern hemisphere solar radio heliograph

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dc.contributor.author Sawant, H. S
dc.contributor.author Fernandes, F. C. R
dc.contributor.author Neri, J. A. C. F
dc.contributor.author Cecatto, J. R
dc.contributor.author Faria, C
dc.contributor.author Stephany, S
dc.contributor.author Rosa, R. R
dc.contributor.author Andrade, M. C
dc.contributor.author Ludke, E
dc.contributor.author Subramanian, K. R
dc.contributor.author Ramesh, R
dc.contributor.author Sundrarajan, M. S
dc.contributor.author Sankararaman, M. R
dc.contributor.author Ananthakrishnan, S
dc.contributor.author Swarup, G
dc.contributor.author Boas, J. W. V
dc.contributor.author Botti, L. C. L
dc.contributor.author Moron, C. E
dc.contributor.author Saito, J. H
dc.contributor.author Karlicky, M
dc.date.accessioned 2009-05-20T13:49:55Z
dc.date.available 2009-05-20T13:49:55Z
dc.date.issued 2002-12
dc.identifier.citation A. Wilson., ed., Solar variability: from core to outer frontiers. The 10th European Solar Physics Meeting, 9 - 14 September 2002, Prague, Czech Republic. ESA SP - 506, Vol. 2, pp. 971 - 974 en
dc.identifier.isbn 92-9092-816-6
dc.identifier.uri http://hdl.handle.net/2248/4480
dc.description.abstract The Brazilian Decimetric Array (BDA) is being developed at National Institute for Space Research (INPE) as an international collaborative program. Initially, the BDA will operate in the tuneable frequency range of 1.2-1.7 GHz. The initial planned baseline for BDA 'T' array is 256×144 m and will be extended to 2.2×1.1 km. In this paper, we present the results of developments concerning the prototype of BDA (PBDA). The PBDA will initially operate in the frequency range of 1.2-1.7 GHz, with a five-antenna array, using 4-meter parabolic dishes with altitude and azimuth mountings and complete tracking capability. The spatial resolution for solar images with the PBDA will be about 3.5 arc-minutes leading to a sensitivity of ≍2×104 mJy/beam for an integration time of 1 sec. The array will be installed at -22°41'19" latitude and 45°0'22" W longitude and it is under operation between 9 and 21 UT for continuous solar flux monitoring. Details of the PBDA system are presented. en
dc.language.iso en en
dc.publisher European Space Agency en
dc.relation.uri http://adsabs.harvard.edu/abs/2002ESASP.506..971S en
dc.subject Radio en
dc.subject Heliograph en
dc.subject Decimetric Wavelengths en
dc.title Southern hemisphere solar radio heliograph en
dc.type Article en


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