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HELAS: the European Helio- and Asteroseismology Network

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Mem. S.A.It. Vol. 80, 276

SAIt 2009 c Memorie

della

HELAS: the European Helio- and Asteroseismology Network

M. P. Di Mauro

INAF-Istituto di Astrofisica Spaziale e Fisica Cosmica, Via del Fosso del Cavaliere 100, I-00133 Roma, Italy, e-mail: mariapia.dimauro@iasf-roma.inaf.it

Abstract. The Helio- and Asteroseismology Network (HELAS) is a Coordinated Action funded for the period 2006-2010 by the FP6-Infrastructure-Programme of the European Commission. INAF is one of the ten partners of HELAS. The objective of HELAS is to co- ordinate European activities in Helio- and Asteroseismology, transfer knowledge and data analysis techniques, and prepare the European research community for important missions in the immediate future.

Key words. Stars: oscillations, asteroseismology – Sun: oscillations, helioseismology

1. Introduction

During the past 40 years, Helioseismology through the careful analysis of the sound waves observed at the surface has become the prime technique to verify the quite com- plex set of mathematical equations and ma- terial properties which describe what we be- lieve the physics of the interior of the Sun to be. In addition, the success of helioseismol- ogy has spurred investigators to extend this diagnostic to other stars which show multi- mode pulsations. This discipline, known as Asteroseismology, opened a new window on the astrophysics research: the possibility to study and to understand the behaviour of other stars by applying the tools and the techniques well developed and used in helioseismology.

European science counts numerous active research groups in the field of Helio- and Asteroseismology. However these groups re-

Send offprint requests to: M. P. Di Mauro

quire networking activities in order to structure and rationalize their efforts.

2. HELAS

The Helio- and Asteroseismology Network HELAS, was established in the 2006 as Coordination Action (CA) funded under the European Commission’s Sixth Framework Programme (FP6). It was created to coordinate activities among those European institutions and organizations that support major research groups in Helio- and Asteroseismology, in or- der to enhance the quality and quantity of these sciences performed in Europe. It offers the unique opportunity to facilitate the exchange of knowledge and the coordination of research in Helio- and Asteroseismology through interna- tional conferences, smaller meetings, staff ex- change and a strong plan for the dissemination of the latest results.

HELAS is led by ten major research groups

in the field from nine European countries:

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Di Mauro: HELAS 277 1. Kiepenheuer-Institut f¨ur Sonnenphysik,

Freiburg, Germany

2. Instituto de Astrof´ısica de Canarias, La Laguna, Tenerife, Spain

3. Department of Applied Mathematics University of Sheffield, Sheffield, U.K.

4. Institut for Fysik og Astronomi, Århus Universitet, Århus, Denmark

5. Centro de Astrofsica da Universidade do Porto, Porto,Portugal

6. Max-Planck-Institut f¨ur Sonnensystemfor- schung, Katlenburg-Lindau, Germany 7. INAF, Istituto Nazionale di Astrofisica,

Roma, Italy

8. Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Leuven, Belgium 9. Instytut Astronomiczny Uniwersytet

Wrocławski, Wrocław, Poland

10. Centre National de la Recherche Scientifique, Observatoire de la Cˆote d’Azur, Nice, France

It is useful to point out that the HELAS activities although coordinated by the ten above partners are extended to all the inter- ested European institutions. The funding of HELAS started on April 1, 2006, and will last until March 31, 2010. Further information can be obtained through the HELAS website http://www.helas-eu.org.

3. Network activities

HELAS, according to the FP6 rules, cannot fund research and development, but supports the coordination of the following activities:

Management: it handles the overall coordina- tion of the consortium, the financial ad- ministration and the interaction with the European Commission.

Forum: it generates and exploits synergies, or- ganizes annual international conferences and manages an internet portal which al- lows the exchange and distribution of soft- wares, data and any other information rele- vant for the field.

Global Helioseismology: it coordinates the distribution of data, methods and tools for global helioseismology.

Local Helioseismology: it aims to create and enlarge the European competences in local Helioseismology.

Asteroseismology: it coordinates the distribu- tion and comparison of observational data, analysis tools, stellar evolution codes and stellar models.

Public outreach: it aims at raising awareness and interest in the field in the general public and at all levels of the educational system.

4. INAF as HELAS partner

The Helio- and Asteroseismology group of INAF, Istituto Nazionale di Astrofisica, which consists of several institutes of astronomy and astrophysics in Italy was established in 2001 with the idea to gather people with comple- mentary skills in the field. The group is in- volved in the study of stellar oscillations with regards to photometric and spectroscopic ob- servations and data analysis, particularly of solar-type, δ Scuti, γ Doradus, sdB and white dwarfs stars. The theoretical works focuses on expertises in the interpretation of the observed oscillation spectra, in particular by the appli- cation and development of helioseismic inver- sion techniques useful to unveil solar and stel- lar internal regions. The team employes its own stellar evolution codes (ATON and FRANEC) with the aim to study the internal structure of the stars in various phases of their evolu- tion. The group is actively involved in sev- eral space stellar missions such as COROT (launched in 2007), Kepler by NASA (launch in 2009) and PLATO by ESA (not yet defi- nitely accepted). The team is also taking part in ADAHELI, which is an ASI solar space mis- sion whose proposal is still in phase A. Further information for the Italian researchers can be obtained through the HELAS Italian website http://www.iasf-roma.inaf.it/helas.

Acknowledgements. This work was supported

by the European Helio- and Asteroseismology

Network (HELAS), a major international collabo-

ration funded by the European Commission’s Sixth

Framework Programme.

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