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Radio Astronomy Centre

National Centre for Radio Astrophysics

Tata Institute of Fundamental Research

        The e-Callisto is an international network of Solar Radio Spectrometers. The hardware and software of Ooty e-Callisto spectrometers were developed by the groups at Institute for Astronomy, ETH Zurich and FHNW Brugg/Windisch, Switzerland.The Radio Astronomy Centre (NCRA-TIFR) at Udhagamandalam(Ooty) maintains two of the spectrometers for observational facility.

* List of Solar bursts detected by Ooty e-Callisto Instruments in 2014 : Data : pdf

* List of Solar bursts detected by Ooty e-Callisto Instruments in 2013 : Data : pdf

*Ooty e-Callisto Data (From Janurary 2014 onwards)

*e-Callisto : Data Site

Selected References :

    * " CALLISTO - A New Concept for Solar Radio Spectrometers", A. O. Benz, C. Monstein & H. Meyer, Solar Phys. 226, 143–151 (2005)

    * "A World-Wide Net of Solar Radio Spectrometers e-CALLISTO", A. O. Benz, C. Monstein, H. Meyer, P. K. Manoharan, R. Ramesh, A. Altyntsev, A. Lara, J. Paez , K.-S. Cho, Earth Moon Planet,DOI: 10.1007/s11038-008-9267-6.

    * “Catalog of dynamic electromagnetic spectra observed with Callisto, Phoenix-3 and ARGOS”, Christian Monstein, Updated 15.12.2013.Journal of the Society of Amateur Radio Astronomers January-February 2013, Vol. 8, p. 25-41.

    * "Callisto spectrum measurements in Ootacamund", Chr. Monstein, P. K. Manoharan and D. Nandagopal, Astronomy and Astrophysics, doi=