Autor: Hari Om Vats, E. M. B. Alonso, A.R.F. Martinon, José Cecatto, F. P. V. Mesquita, J.A.C.F. Neri, Francisco Carlos Fernandes, Reinaldo R. Rosa, K. R. Subramanian, C. Faria, V.A. Portezani, J. H. A. Sobral, Hanumant S. Sawant
Rok vydání: 2001
Předmět:
Zdroj: Solar Physics. 200:167-176
ISSN: 0038-0938
DOI: 10.1023/a:1010366311616
Popis: Digital, decimetric (200–2500 MHz) Brazilian Solar Spectroscope (BSS) with high time (10–1000 ms) and frequency (1–10 MHz) resolution is in regular operation since April, 1998, at National Space Research Institute (INPE) at Sao Jose dos Campos, Brazil. BSS operates in conjunction with a 9-m diameter polar mounted antenna. It allows to select suitable observing frequency range, frequency and time resolutions and data can be digitized up to 100 channels. BSS has capabilities of quasi-real time display of the ongoing dynamic spectra of the solar activity that enables the observer to modify observational parameters so as to suit a specific type of activity such as spikes and improve the quality of data acquisition and storage. Minimum detectable flux density of the spectroscope, for different combinations of the observational parameters, is ∼3 s.f.u. Observations are carried out routinely from 11 UT to 19 UT. Necessary software for data acquisition and reductions has been developed in IDL 5.3 environment. Data are available in FITS and ASCII formats. Absolute timing accuracy of the station is less than 3 ms. Here, we present examples of the bursts which have been recorded by BSS and available display facilities.
Databáze: OpenAIRE
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