A World-Wide Net of Solar Radio Spectrometers: e-CALLISTO

Details A World-Wide Net of Solar Radio Spectrometers: e-CALLISTO A World-Wide Net of Solar Radio Spectrometers: e-CALLISTO

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009em%26p..104..277b&link_type=abstract

Earth, Moon, and Planets, Volume 104, Issue 1-4, pp. 277-285

Physics

4

Solar Radio Emission, Radio Spectrometer, International Science Cooperation, Global Network, Space Weather, International Heliospheric Year

Scientific paper

Radio spectrometers of the CALLISTO type to observe solar flares have been distributed to nine locations around the globe. The instruments observe automatically, their data is collected every day via internet and stored in a central data base. A public web-interface exists through which data can be browsed and retrieved. The nine instruments form a network called e-CALLISTO. It is still growing in the number of stations, as redundancy is desirable for full 24 h coverage of the solar radio emission in the meter and low decimeter band. The e-CALLISTO system has already proven to be a valuable new tool for monitoring solar activity and for space weather research.

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