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Physique Solaire et Stellaire
French
Cette mission (NASA, lancée en 2009), dans la lignée de CoRoT, combine elle aussi sismologie des étoiles et recherche d’exo-planètes. L’équipe participe activement à l’exploitation des données.
Contact: T. Appourchaux
Illustration du projet:
The CoRoT target HD 49933 II. Comparison of theoretical mode amplitudes with observations
Fri, 06/06/2014 - 15:37
webadm
Astronomy & Astrophysics, vol. 509. 2010.
Reflection Driven MHD Turbulence in the Solar Atmosphere and Wind
Fri, 06/06/2014 - 15:37
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Earth Moon and Planets, vol. 104. pp. 121-125, 2009.
The SWAP EUV Imaging Telescope Part I: Instrument Overview and Pre-Flight Testing
Fri, 06/06/2014 - 15:37
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Solar PhysicsSolar Physics. p. 217, 2012.
HYDROGEN Ly alpha AND Ly beta RADIANCES AND PROFILES IN POLAR CORONAL HOLES
Fri, 06/06/2014 - 15:37
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Astrophysical Journal Letters, vol. 703. pp. L152-L156, 2009.
Constructing a One-solar-mass Evolutionary Sequence Using Asteroseismic Data from Kepler
Fri, 06/06/2014 - 15:37
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The Astrophysical Journal Letters, vol. 740. p. L2, 2011.
Weak turbulence in two-dimensional magnetohydrodynamics
Fri, 06/06/2014 - 15:37
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Physical Review EPhysical Review E, vol. 87. p. 33103, 2013.
RADIUS DETERMINATION OF SOLAR-TYPE STARS USING ASTEROSEISMOLOGY: WHAT TO EXPECT FROM THE KEPLER MISSION
Fri, 06/06/2014 - 15:37
webadm
Astrophysical Journal, vol. 700. pp. 1589-1602, 2009.
TURBULENCE IN THE SUB-ALFVENIC SOLAR WIND DRIVEN BY REFLECTION OF LOW-FREQUENCY ALFVEN WAVES
Fri, 06/06/2014 - 15:37
webadm
Astrophysical Journal Letters, vol. 700. pp. L39-L42, 2009.
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