Solar radio astronomical big data classification
Lecture Notes in Computer Science (including subseries Lecture Notes in Artificial Intelligence and Lecture Notes in Bioinformatics), ISSN: 1611-3349, Vol: 9576, Page: 126-133
2016
- 7Captures
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Example: if you select the 1-year option for an article published in 2019 and a metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019. If you select the 3-year option for the same article published in 2019 and the metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019, 2018 and 2017.
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Metrics Details
- Captures7
- Readers7
Conference Paper Description
The Solar Broadband Radio Spectrometer (SBRS) monitors the solar radio busts all day long and produces solar radio astronomical big data foranalysis every day, which usually have been accumulated in mass images for scientific study over decades. In the observed mass data, burst events are rare and always along with interference, so it seems impossible to identify whether the mass data contain bursts or not and figure out which type of burst it is by manual operation timely. Therefore, we take advantage of high performance computing and machine learning techniques to classify the huge volume astronomical imaging data automatically. The professional line of multiple NVIDIA GPUs has been exploited to deliver 78x faster parallel processing power for high performance computing of the astronomical big data, and neural networks have been utilized to learn the representations of the solar radio spectra. Experimental results have demonstrated that the employed network can effectively classify a solar radio image into the labeled categories. Moreover, the processing time is dramatically reduced by exploring GPU parallel computing environment.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=84979221624&origin=inward; http://dx.doi.org/10.1007/978-3-319-32557-6_13; http://link.springer.com/10.1007/978-3-319-32557-6_13; http://link.springer.com/content/pdf/10.1007/978-3-319-32557-6_13; https://dx.doi.org/10.1007/978-3-319-32557-6_13; https://link.springer.com/chapter/10.1007/978-3-319-32557-6_13
Springer Science and Business Media LLC
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