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Proceedings Paper

A complete solar eruption activity processing tool with robotization and real time (II)
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Paper Abstract

Intense solar active events have made significant impacts on the modern high technology system and living environment of human being, therefore solar activities forecast and space weather forecast are getting more and more attention. Meanwhile, data volume acquisitioned by solar monitor facility is growing larger and larger due to the requirement of multiple dimensions observation and high temporal and spatial resolution. As staffs of a solar monitor data producer, we are encouraged to adopt new techniques and methods to provide valuable information to solar activities forecast organization and the other related users, and provide convenient products and tools to the users. In the previous paper “A complete solar eruption activities processing tool with robotization and real time (I)”, we presented a fully automatic and real time detecting architecture for different solar erupt activities. In this paper, we present new components of new data sets in the architecture design, latest progresses on automatic recognition of solar flare, filament and magnetic field, and a newly introduced method with which solar photospheric magnetic nonpotentiality parameters are processed in real time, then its result directly can be used in solar active forecast.

Paper Details

Date Published: 18 July 2014
PDF: 7 pages
Proc. SPIE 9152, Software and Cyberinfrastructure for Astronomy III, 915222 (18 July 2014); doi: 10.1117/12.2057246
Show Author Affiliations
Ganghua Lin, National Astronomical Observatories (China)
Cui Zhao, National Astronomical Observatories (China)
Xiao Yang, National Astronomical Observatories (China)

Published in SPIE Proceedings Vol. 9152:
Software and Cyberinfrastructure for Astronomy III
Gianluca Chiozzi; Nicole M. Radziwill, Editor(s)

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