Solaris is a scientific and technological project aimed at the development of a smart Solar monitoring system at high radio frequencies, based on single-dish imaging techniques. It combines the implementation of dedicated and interchangeable high-frequency receivers on existing small single-dish radio telescope systems (1.5/2.6m class) available in our laboratories and in Antarctica, to be adapted for Solar observations. Solaris can perform Solar imaging observations nearly 20h/day during Antarctic summer with optimal sky opacity, and it will be the only Solar facility offering continuous monitoring at 100GHz. In perspective, our system could be implemented also in the Northern hemisphere to offer unprecedented Solar radio monitoring and imaging for the whole year.
KEYWORDS: Solar processes, Data archive systems, Polarization, Space weather, Polarimetry, Physics, Data modeling, Coronagraphy, Satellite navigation systems, Observatories
The TSRS was a set of two multi-channel solar radio polarimeters which performed continuous surveillance of the decimetric and metric coronal radio emissions with high time resolution. TSRS was operational in Trieste (Italy) under the management of the INAF Astronomical Observatory of Trieste from 1969 to 2010 when a lightning stroke irreparably compromised its operations. Starting from that moment, all the services related to it, including the archive system, were abandoned due to lack of funds and resources. An Heritage Archive (TSRS-HA) has been preserved with the available digitized data and this contribution describes how it was planned to refurbish archive and service for such a heritage resource following current common FAIR principles adherence and new technologies.
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