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IMPACT SWEA electron measurements and the temporal evolution of the solar wind

SWG 2010 Spring, Dublin, Ireland. IMPACT SWEA electron measurements and the temporal evolution of the solar wind. Andrea Opitz CESR, Toulouse, France for the SWEA team and its supporters. SWEA core density proxy. SWEA status reported by J-A. Sauvaud and J. Luhmann

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IMPACT SWEA electron measurements and the temporal evolution of the solar wind

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  1. SWG 2010 Spring, Dublin, Ireland IMPACT SWEAelectron measurements and the temporal evolution of the solar wind Andrea Opitz CESR, Toulouse, France for the SWEA team and its supporters

  2. SWEA core density proxy SWEA status reported by J-A. Sauvaud and J. Luhmann • High energy excellent measurements: PADs, Q, etc. • SWEA data available at http://stereo.cesr.fr • Low energy solar wind electrons suppressed < 45 eV • No core distribution SW electron core reconstruction from secondary electrons • Secondaries produced in instrument are unveiled • Secondaries depend on density of SW electrons arriving on SWEA • Derive SW electron density proxy from secondary electrons Fedorov, Opitz, Sauvaud et al. 2010 submitted at SSR

  3. SWEA core density proxy Ne: SWEA by CESR, Np: PLASTIC by UNH

  4. STEREO timelag STA STB PLASTIC velocity SWEA density Opitz et al. 2009, SolPhys

  5. SWEA electron core density Opitz et al. 2010a, submitted at Solar Physics

  6. Temporal evolution of the solar wind Opitz et al. 2009a, Solar Physics PLASTIC velocity  0.5 day: ~0.95 2 days: ~0.85 Opitz et al. 2010a, submitted at Sol. Phys. SWEA density  0.5 day: ~0.80 2 days: ~0.65

  7. SW temporal evolution

  8. SW prediction for heliosphere August 2007 Opitz et al. 2009, SolPhys Opitz et al. 2010b, submitted at SolPhys

  9. References • Fedorov A., Opitz A., Sauvaud J-A., Luhmann J. G., Curtis D. W., and Larson D. E.SWEA in-flight properties. Reconstruction of the SWEA transmission function by numerical simulation and data analysis Space Science Review, submitted, 2010 • Opitz A., Karrer R., Wurz P., Galvin A. B., Bochsler P., et al.Temporal evolution of the solar wind bulk velocity at solar minimum by correlating the STEREO A and B PLASTIC measurementsSolar Physics, vol. 256, p365 , 2009 • Opitz A., Sauvaud J-A., Fedorov A., Wurz P., Luhmann J. G., Lavraud B., Russell C. T., Kellogg P., Briand C., Henri P., Malaspina D. M., Louarn P., Curtis D. W., Penou E., Karrer R., Galvin A. B., Larson D. E., Dandouras I., and Schroeder P. Temporal evolution of the solar wind electron core density at solar minimum by correlating the STEREO A and B SWEA measurements Solar Physics, submitted, 2010a • Opitz A., Fedorov A., Wurz P., Szego K., Sauvaud J-A., Karrer R., Galvin A. B., Barabash S., and Ipavich F. Solar wind bulk velocity throughout the inner heliosphere from multi-spaceraft measurementsSolar Physics, submitted, 2010b • Sauvaud J-A., Larson D., Aoustin C., Curtis D., Medale J-L., Fedorov A., Rouzaud J., Luhmann J., Moreau T., Schroeder P., Louarn P., Dandouras I., and Penou E.The IMPACT Solar Wind Electron Analyzer (SWEA) Space Sci. Rev., vol. 136, p227, 2008

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