RĂ©sultats 1 - 10 sur un total de 264
Kassi Samir, Wang Le, Campargue Alain.
Temperature dependence of the absorption spectrum of methane by high sensitivity laser spectroscopy between 1.27 and 1.71 micron at 80 K and 300 K. Importance of the CH3D contribution in the 1.58 micron transparency window..
EGU 2010, 2010, Vienne, Austria. pp.9809.
Référence ADS : 2010EGUGA..12.9809K
Référence HAL : hal-01005754
Langlois M., Vigan Arthur, Dohlen K., Moutou C., Mouillet D., Wildi F., Boccaletti A..
Impact of calibration on extrasolar planets direct imaging with IRDIS, the infrared dual-imaging camera and spectrograph for SPHERE.
SPIE Astronomical Telescopes + Instrumentation, Jul 2010, San Diego, United States. pp.773512, ⟨10.1117/12.857194⟩.
Référence DOI : 10.1117/12.857194
Référence ADS : 2010SPIE.7735E..12L
Référence HAL : hal-02118209
Cornia A., Mugnier L. M., Mouillet D., Vigan Arthur, Eggenberger A., Rousset G., Boccaletti A., Carbillet M., Dohlen K., Fusco T., Carson J., Montagnier G..
Optimal method for exoplanet detection by spectral and angular differential imaging.
SPIE Astronomical Telescopes + Instrumentation, Jul 2010, San Diego, United States. pp.77361E, ⟨10.1117/12.856404⟩.
Référence DOI : 10.1117/12.856404
Référence ADS : 2010SPIE.7736E..1EC
Référence HAL : hal-02118211
Vigan Arthur, Moutou C., Langlois M., Mouillet D., Dohlen K., Boccaletti A., Carbillet M., Smith I., Ferrari Anthony, Mugnier L., Thalmann C., Mclean Ian, Ramsay Suzanne, Takami Hideki.
Comparison of methods for detection and characterization of exoplanets with SPHERE/IRDIS.
SPIE Astronomical Telescopes + Instrumentation, Jul 2010, San Diego, United States. pp.77352X, ⟨10.1117/12.856701⟩.
Référence DOI : 10.1117/12.856701
Référence ADS : 2010SPIE.7735E..2XV
Référence HAL : hal-02118214
Bommier VĂ©ronique, Degl'Innocenti Egidio Landi, Schmieder Brigitte, Gelly Bernard.
Vector magnetic field and vector current density in and around the δ-spot NOAA 10808.
The Physics of Sun and Star Spots, IAU Symposium 273, Aug 2010, Ventura, United States. pp.338-338, ⟨10.1017/S1743921311015493⟩.
Référence DOI : 10.1017/S1743921311015493
Référence HAL : hal-02382991
Guo Y., Schmieder B., Démoulin P., Wiegelmann T., Aulanier G., Török T., Bommier V..
A filament supported by different magnetic field configurations.
The Physics of Sun and Star Spots, IAU Symposium 273, Aug 2010, Ventura (Californie), United States. pp.328-332, ⟨10.1017/S174392131101547X⟩.
Référence DOI : 10.1017/S174392131101547X
Référence HAL : hal-02383002
Bommier V..
The Quiet Sun Magnetic Field Structure Derived from a Full Vector Determination.
Solar Polarization 6, May 2010, Haleakala Maui (HawaĂŻ), United States. pp.471.
Référence ADS : 2011ASPC..437..471B
Référence HAL : hal-02383101
Alexandrova O., Saur J., Lacombe C., Mangeney A., Schwartz S. J., Mitchell J., Grappin Roland, Robert Patrick.
Solar wind turbulent spectrum from MHD to electron scales.
TWELFTH INTERNATIONAL SOLAR WIND CONFERENCE, 2010, Saint-Malo, France. pp.144-147, ⟨10.1063/1.3395821⟩.
Référence DOI : 10.1063/1.3395821
Référence HAL : hal-02793780
Bommier V..
The magnetic field of the solar plasma.
37th Conference on Plasmas Physics, European Physical Society, Jun 2010, Dublin, Ireland.
Référence HAL : hal-02907096
Bommier V..
Magnetic field measurements with THEMIS.
EST-France 2010 International Workshop, Programme National "Soleil-Terre" du C.N.R.S., May 2010, Meudon, France.
Référence HAL : hal-02907982
