Organization of a Unified Data Archive and Accessories for Processing Solar Images

Part of the Astrophysics and Space Science Library book series (ASSL, volume 400)


The orbital solar observatory CORONAS-F was launched in late July 2001. A vast database from 12 onboard instrumental complexes was accumulated for 3 years of the satellite operation time. The data processing information was displayed on the project site The bulk of data received from CORONAS-F amounted to 100 MB/day. On-line processing of such amounts of data was quite a challenge. The preprocessed CORONAS-F data were, then, subjected to additional processing by the principal investigators at the corresponding institutions, including the calibration, space-time binding, clearing, etc. The resulting data are stored at the participant institutions in the form of profiles, spectrograms, and images. The stored “raw” data are the main source of reliable information for further investigations, but they usually need further processing to be visualized. Besides, a full cycle of processing of the scientific data takes much time and can even drag on for years under financial stringency and shortage of personnel. The final information is stored at different institutions that do not possess unified means of access, analysis, and visualization of data. This hampers significantly the use of the entire database by individual researchers.


Entire Database Solar Image Virtual Laboratory Participant Institution Unify Means 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Copyright information

© Springer-Verlag Berlin Heidelberg 2014

Authors and Affiliations

  1. 1.Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation RAS (IZMIRAN)MoscowRussia

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