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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
Affiliation:
LESIA, Observatoire de Paris, CNRS, UPMC, Universit Paris-Diderot, 5 place Jules Janssen, 92195 Meudon, France email: xavier.bonnin@obspm.fr, nicolas.fuller@obspm.fr, christian.renie@obspm.fr, jean.aboudarham@obspm.fr, baptiste.ceconni@obspm.fr
Nicolas Fuller
Affiliation:
LESIA, Observatoire de Paris, CNRS, UPMC, Universit Paris-Diderot, 5 place Jules Janssen, 92195 Meudon, France email: xavier.bonnin@obspm.fr, nicolas.fuller@obspm.fr, christian.renie@obspm.fr, jean.aboudarham@obspm.fr, baptiste.ceconni@obspm.fr
Christian Renié
Affiliation:
LESIA, Observatoire de Paris, CNRS, UPMC, Universit Paris-Diderot, 5 place Jules Janssen, 92195 Meudon, France email: xavier.bonnin@obspm.fr, nicolas.fuller@obspm.fr, christian.renie@obspm.fr, jean.aboudarham@obspm.fr, baptiste.ceconni@obspm.fr
Jean Aboudarham
Affiliation:
LESIA, Observatoire de Paris, CNRS, UPMC, Universit Paris-Diderot, 5 place Jules Janssen, 92195 Meudon, France email: xavier.bonnin@obspm.fr, nicolas.fuller@obspm.fr, christian.renie@obspm.fr, jean.aboudarham@obspm.fr, baptiste.ceconni@obspm.fr
Baptiste Cecconi
Affiliation:
LESIA, Observatoire de Paris, CNRS, UPMC, Universit Paris-Diderot, 5 place Jules Janssen, 92195 Meudon, France email: xavier.bonnin@obspm.fr, nicolas.fuller@obspm.fr, christian.renie@obspm.fr, jean.aboudarham@obspm.fr, baptiste.ceconni@obspm.fr
Robert D. Bentley
Affiliation:
MSSL, University College London, Hombury St. Mary, Dorking, Surrey RH5 6NT, U.K. email: rdb@mssl.ucl.ac.uk
André Csillaghy
Affiliation:
Institute of 4D Technologies, FHNW, Steinackerstrass 5, CH-5210 Windisch, Switzerland email: andre.csillaghy@fhnw.ch
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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, . . .

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2013 

References

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