A World-Wide Net of Solar Radio Spectrometers: e-CALLISTO
A World-Wide Net of Solar Radio Spectrometers: e-CALLISTO
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DOI：
10.1007/s11038-008-9267-6
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发表时间：
2009-01
期刊：
影响因子：
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通讯作者：
A. Benz;C. Monstein;H. Meyer;P. Manoharan;R. Ramesh;A. Altyntsev;A. Lara;J. Páez;Kyung-Suk Cho-Kyu
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文献类型：
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作者：
A. Benz;C. Monstein;H. Meyer;P. Manoharan;R. Ramesh;A. Altyntsev;A. Lara;J. Páez;Kyung-Suk Cho-Kyu
用于观测太阳耀斑的CALLISTO型无线电光谱仪已分布在全球九个地点。仪器自动观测，数据每天通过互联网收集并存储在中央数据库中。存在一个公共网络接口，通过它可以浏览和检索数据。这九种仪器组成了一个叫做e-CALLISTO的网络。台站的数量仍在增长，因为在米和低分米波段对太阳射电发射的24小时全覆盖是需要冗余的。e-CALLISTO系统已经被证明是监测太阳活动和空间天气研究的一个有价值的新工具。
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.