Published April 2005
| Version v1
Conference paper
The magnetism of the solar interior for a complete MHD solar vision
Creators
- Turck-Chièze, S.
- Appourchaux, Thierry
- Ballot, J.
- Berthomieu, G.
- Boumier, P.
- Brun, A.
- Cacciani, A.
- Christensen-Dalsgaard, J.
- Corbard, T.
- Couvidat, S.
- Eff-Darwich, A.
- Dintrans, B.
- Fossat, E.
- Garcia, R.
- Gelly, B.
- Gizon, L
- Gough, D.
- Jimenez, A.
- Jimenez-Reyes, S.
- Kosovishev, A.
- Lambert, P.
- Lopes, I.
- Martic, Milena
- Mathis, S.
- Meunier, N.
- Nghiem, P.
- Palle, P.
- Piau, L.
- Provost, J.
- Rieutord, M.
- Robillot, J.
- Rodier, T.
- Roxburgh, I.
- Rozelot, J.
- Solanki, S.
- Talon, S.
- Thompson, M.
- Thuillier, Gérard
- Vauclair, S.
- Zahn, J.-P.
Contributors
Others:
- Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée (DAPNIA) ; Commissariat à l'énergie atomique et aux énergies alternatives (CEA)
- Institut d'astrophysique spatiale (IAS) ; Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)
- Observatoire de la Côte d'Azur ; COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)
- Dipartimento di Fisica [Roma La Sapienza] ; Università degli Studi di Roma "La Sapienza" = Sapienza University [Rome] (UNIROMA)
- Department of Physics and Astronomy [Aarhus] ; Aarhus University [Aarhus]
- Hansen Experimental Physics Lab [Stanford] (HEPL) ; Stanford University
- Departamento de Astrofísica [La laguna] ; Universidad de La Laguna [Tenerife - SP] (ULL)
- Observatoire Midi-Pyrénées (OMP) ; Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3) ; Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France
- Laboratoire Universitaire d'Astrophysique de Nice (LUAN) ; Université Nice Sophia Antipolis (1965 - 2019) (UNS) ; COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
- Max-Planck-Institut
- Institute of Astronomy [Cambridge] ; University of Cambridge [UK] (CAM)
- Instituto Superior Técnico ; Technical University of Lisbon
- Service d'aéronomie (SA) ; Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
- Observatoire de Paris - Site de Meudon (OBSPM) ; Observatoire de Paris ; Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)
- Department of Astronomy and Astrophysics [Chicago] ; University of Chicago
- Observatoire Bordeaux ; Université Sciences et Technologies - Bordeaux 1
- Queen Mary University of London (QMUL)
- Département de Physique [Montréal] ; Université de Montréal (UdeM)
- University of Sheffield [Sheffield]
- F. Favata
- J. Sanz-Forcada
- Á. Giménez (eds)
Description
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 dynam- ics 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 understand the com- plex 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.
Abstract
International audienceAdditional details
Identifiers
- URL
- https://hal.archives-ouvertes.fr/hal-03598321
- URN
- urn:oai:HAL:hal-03598321v2