eCallisto radiospectrograms

The CALLISTO spectrometer is a programmable heterodyne receiver built in the framework of IHY2007 and ISWI by former Radio and Plasma Physics Group (PI Christian Monstein) at ETH Zurich, Switzerland. This application provides access to the data from these receivers that are installed on radio antennas around the globe. The data are used for the identification of radio bursts as indications of Solar phenomena driving Space Weather.


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eCallisto

The CALLISTO spectrometer is a programmable heterodyne receiver built in the framework of IHY2007 and ISWI by former Radio and Plasma Physics Group (PI Christian Monstein) at ETH Zurich, Switzerland. The main applications are observation of solar radio bursts and rfi-monitoring for astronomical science, education and outreach. This product provides access to a world-wide collection of such spectrometers, called the eCallisto network. The product includes RAW data and quicklook images.

Many CALLISTO instruments have already been deployed, including: 5 spectrometers in India (2 in Ooty, 1 in Gauribidanur, 1 in Pune, 1 in Ahmedabad), 1 in Badary near Irkutsk, Russian Federation, 2 in South Korea, 3 Australia (Perth, Melbourne and Heathcote), 2 in Hawaii, 2 in Mexico, 1 in Costa Rica, 2 in Brazil, 3 in Mauritius, 5 in Ireland, 1 in Czech Republic, 2 in Mongolia, 4 in Germany, 2 in Alaska, 2 in Kazakhstan, 1 in Cairo, 1 in Nairobi, 1 in Sri Lanka, 3 in Trieste, 1 in Hurbanovo/Slovakia, 2 in Belgium, 2 in Finland, 8 in Switzerland, 1 in Sardinia, 4 in Spain, 5 in Malaysia, 3 in Indonesia, 1 in Scotland/UK 1 in Roztoky/Slovakia, 1 in Peru, 1 in Rwanda, 1 in Pakistan, 2 in Denmark, 1 in Japan, 1 in South Africa, 2 in Greenland, 2 in Austria and 1 in Uruguay. Through the IHY/UNBSSI and ISWI instrument deployment program, CALLISTO is able to continuously observe the solar radio spectrum for 24h per day throughout the year. All Callisto spectrometers together form the e-Callisto network. Callisto in addition is dedicated to radio-monitoring within its frequency range with 13,200 channels per spectrum. The frequency range can be expanded to any range by switching-in a heterodyne up- or a down-converter. Instrument deployment including education and training of observers was financially supported by SNF, SSAA (Swiss Society for Astrophysics and Astronomy), NASA, Institute for Astronomy and North-South Center of ETH Zurich and a few private sponsors.

For more information please visit this page: http://www.e-callisto.org/

If you would like to use the API, please visit this webpage here:

Link: Swagger API

The top menu navigation bar allows the user to browse through the products (across the different "Solar Weather" providers) as follows: