Solar v - TAUP 2009 - Infn

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10 Megaton:ICECUBE ν e ν μ Fargion D.-TAUP D. TAUP-01 01-07 07-2009 2009-Rome Rome 22 ν
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Page 1 and 2: Underground megatons detectors :Sol
Page 3 and 4: The lepton thresholds Fargion D.-TA
Page 5 and 6: (1987) Supernova Neutrinos Expected
Page 7 and 8: From half century ago..1956 Neutron
Page 9 and 10: Flare-Supernova Flare Supernova 198
Page 11 and 12: Fargion D.-TAUP D. TAUP-01 01-07 07
Page 13 and 14: Why so much interest for the 20° J
Page 15 and 16: The neutral-pion neutral pion signa
Page 17 and 18: SK ν e ν μ ν τ Fargion D.-TAUP
Page 19 and 20: Correct cross section Fargion D.-TA
Page 21: ν e 5 MEGATON TITAND ν μ ν τ F
Page 25 and 26: SK Anti ν e after in SK ν e ν μ
Page 27 and 28: 12 MeV solar ν The low energy ν-e
Page 29 and 30: 603 MeV atmospheric muon ν Note sh
Page 31 and 32: Highest energetic solar particles F
Page 33 and 34: A first SK Tau ν candidate event (
Page 35 and 36: Probability Meaning Fargion D.-TAUP
Page 37 and 38: Fargion D.-TAUP D. TAUP-01 01-07 07
Page 39 and 40: Thank You for the attention Fargion
Page 41 and 42: Present -Future Future Neutrino Det
Page 43 and 44: Solar Standard Model: a noisy neutr
Page 45 and 46: Neutron and Gamma…and Neutrinos?
Page 47: Neutrino muon before mixing Fargion

Solar v - TAUP 2009 - Infn

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