Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/4480
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DC Field | Value | Language |
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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 |
Appears in Collections: | IIAP Publications |
Files in This Item:
File | Description | Size | Format | |
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Southern hemisphere solar radio heliograph | 430.41 kB | Adobe PDF | View/Open |
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