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Status report on SW & Analysis from country xx

Status report on SW & Analysis from country xx. Institutions. list of Universities / Research centers in the country. Institution INFN and Univ. Milano-Bicocca. Composition of the group : manpower for analysis in 2010/2011 Staff : M. Boschini, D. Grandi, M. Gervasi,

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Status report on SW & Analysis from country xx

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  1. Status report on SW & Analysis from country xx

  2. Institutions • list of Universities / Research centers in the country

  3. Institution INFN and Univ. Milano-Bicocca • Composition of the group : manpower for analysis in 2010/2011 Staff : M. Boschini, D. Grandi, M. Gervasi, P.G. Rancoita Post- Doc : C. Consolandi, M. Tacconi PhD students: S. Della Torre Graduate students : D. Rozza, S. Miliano

  4. Institution INFN and Univ. Milano-Bicocca • Current Activities in SW/Analysis • DT • MC Remote production • RAW data DT and storage (CNAF) • MC DT from remote sites CERN • AMS software Web Pages • Re-organization and maintenance • SOCC • Data handling

  5. Institution INFN and Univ. Milano-Bicocca • Current Activities in SW/Analysis Analysis Modulation of antiproton-proton ratio Modulation of positron-electron ratio Tools development: Magnetosphere Tracking for primary and secondary CRs Heliospheremodulationforleptons, protons and ions

  6. Relevant results and on-going activities Modulated Ratio for E < 10 GeV AMS-01 data (Aguilar et. al. 2007) PAMELA data (Adriani et. al. 2008) A> 0 A< 0

  7. A< 0 A> 0

  8. Proton modulation A> 0

  9. Example of primary proton spectrum prediction (January 2012) at 1 AU A< 0

  10. Interests and planning for Y2011 • DT • Remote MC production • DT from NASA to CERN • RAW data CNAF storage • Sub sample Reconstruction • Framework for remote analysis (@CNAF) • Remote analysis

  11. Interests and planning for Y2011 • AMS-02 data • Electrons, positrons and Heliosphere modulation • Proton, antiproton and Magnetosphere backtracking and Heliopshere modulation • Magnetosphere backtracking of electrons, protons and nuclei • Heliosphere modulation of p, anti-p, e-, e+, nuclei • Solar modulation study with p and e- spectra vs time

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