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The Heliophysics Feature Catalogue, a tool for the study of solar features

Published online by Cambridge University Press:  06 January 2014

Xavier Bonnin ,
Nicolas Fuller ,
Christian Renié ,
Jean Aboudarham ,
Baptiste Cecconi ,
Robert D. Bentley  and
André Csillaghy
Xavier Bonnin
Affiliation:
LESIA, Observatoire de Paris, CNRS, UPMC, Universit Paris-Diderot, 5 place Jules Janssen, 92195 Meudon, France email: [email protected], [email protected], [email protected], [email protected], [email protected]
Nicolas Fuller
Affiliation:
LESIA, Observatoire de Paris, CNRS, UPMC, Universit Paris-Diderot, 5 place Jules Janssen, 92195 Meudon, France email: [email protected], [email protected], [email protected], [email protected], [email protected]
Christian Renié
Affiliation:
LESIA, Observatoire de Paris, CNRS, UPMC, Universit Paris-Diderot, 5 place Jules Janssen, 92195 Meudon, France email: [email protected], [email protected], [email protected], [email protected], [email protected]
Jean Aboudarham
Affiliation:
LESIA, Observatoire de Paris, CNRS, UPMC, Universit Paris-Diderot, 5 place Jules Janssen, 92195 Meudon, France email: [email protected], [email protected], [email protected], [email protected], [email protected]
Baptiste Cecconi
Affiliation:
LESIA, Observatoire de Paris, CNRS, UPMC, Universit Paris-Diderot, 5 place Jules Janssen, 92195 Meudon, France email: [email protected], [email protected], [email protected], [email protected], [email protected]
Robert D. Bentley
Affiliation:
MSSL, University College London, Hombury St. Mary, Dorking, Surrey RH5 6NT, U.K. email: [email protected]
André Csillaghy
Affiliation:
Institute of 4D Technologies, FHNW, Steinackerstrass 5, CH-5210 Windisch, Switzerland email: [email protected]
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Abstract

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The behavior of filaments and prominences during the Solar Cycle is a signature of Sun's activity. It is therefore important to follow their evolution during the cycle, in order to be able to associate it with the various phases of the Solar Cycle as well as with other Solar features or events. The virtual observatory HELIO provides information that can be used for such studies, especially its Heliophysics Feature Catalogue gives a unique access to the description of various features during around one cycle. Features available are: filaments, prominences, photospheric and coronal active regions, coronal radio emission, type III radio bursts, coronal holes and sunspots. Web interfaces allow the user to query data for these features. Useful information can also be shared with other HELIO services, such as Heliophysics Event Catalogue, which provides access to dozens of tables of events such as flares, CMEs, . . .

Keywords

Solar featuresAutomatic recognitionImage processingDatabaseData miningVirtual observatory
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S300: Nature of Prominences and their role in Space Weather , June 2013 , pp. 512 - 514
Copyright
Copyright © International Astronomical Union 2013 

References

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