The magnetism of the solar interior for a complete MHD solar vision

S. Turck-Chièze, T. Appourchaux, J. Ballot, G. Berthomieu, P. Boumier, A. S. Brun, A. Cacciani, J. Christensen-Dalsgaard, T. Corbard, S. Couvidat, A. Eff-Darwich, B. Dintrans, E. Fossat, R. A. Garcia, B. Gelly, L. Gizon, D. Gough, A. Jimenez, S. Jimenez-Reyes, A. KosovishevP. Lambert, I. Lopes, M. Martic, S. Mathis, N. Meunier, P. A. Nghiem, P. Palle, L. Piau, J. Provost, M. Rieutord, J. M. Robillot, T. Rodier, I. Roxburgh, J. P. Rozelot, S. Solanki, S. Talon, M. Thompson, G. Thuillier, S. Vauclair, J. P. Zahn

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

The solar magnetism is no more considered as a purely superficial phenomenon. The SoHO community has shown that the length of the solar cycle depends on the transition region between radiation and convection. Nevertheless, the internal solar (stellar) magnetism stays poorly known. Starting in 2008, the American instrument HMI/SDO and the European microsatellite PICARD will enrich our view of the Sun-Earth relationship. Thus obtaining a complete MHD solar picture is a clear objective for the next decades and it requires complementary observations of the dynamics of the radiative zone. For that ambitious goal, space prototypes are being developed to improve gravity mode detection. The Sun is unique to progress on the topology of deep internal magnetic fields and to nderstand the complex mechanisms which provoke photospheric and coronal magnetic changes and possible longer cycles important for human life. We propose the following roadmap in Europe to contribute to this "impressive" revolution in Astronomy and in our Sun-Earth relationship: SoHO (1995-2007), PI-CARD (2008-2010), DynaMICS (2009-2017) in parallel to SDO (2008-2017) then a world-class mission located at the L1 orbit or above the solar poles.

Original languageEnglish (US)
Title of host publicationProceedings of the 39th ESLAB Symposium
Subtitle of host publicationTrends in Space Science and Cosmic Vision 2020
Pages193-202
Number of pages10
Edition588
StatePublished - 2005
Event39th ESLAB Symposium: Trends in Space Science and Cosmic Vision 2020 - Noordwijk, Netherlands
Duration: Apr 19 2005Apr 21 2005

Publication series

NameEuropean Space Agency, (Special Publication) ESA SP
Number588
ISSN (Print)0379-6566

Other

Other39th ESLAB Symposium: Trends in Space Science and Cosmic Vision 2020
CountryNetherlands
CityNoordwijk
Period4/19/054/21/05

Keywords

  • Celestial mechanics
  • General relativity
  • Gravitational moments
  • Solar magnetism
  • Solar rotation
  • Sun

ASJC Scopus subject areas

  • Aerospace Engineering
  • Space and Planetary Science

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  • Cite this

    Turck-Chièze, S., Appourchaux, T., Ballot, J., Berthomieu, G., Boumier, P., Brun, A. S., Cacciani, A., Christensen-Dalsgaard, J., Corbard, T., Couvidat, S., Eff-Darwich, A., Dintrans, B., Fossat, E., Garcia, R. A., Gelly, B., Gizon, L., Gough, D., Jimenez, A., Jimenez-Reyes, S., ... Zahn, J. P. (2005). The magnetism of the solar interior for a complete MHD solar vision. In Proceedings of the 39th ESLAB Symposium: Trends in Space Science and Cosmic Vision 2020 (588 ed., pp. 193-202). (European Space Agency, (Special Publication) ESA SP; No. 588).