Presentation is loading. Please wait.

Presentation is loading. Please wait.

2D-IDAPP meeting Valeria Di Felice University of Rome Tor Vergata Tutor: Prof. Piergiorgio Picozza Ferrara, 3-4 May 2007.

Published byAdrian Hahn Modified over 10 years ago

Similar presentations

Presentation on theme: "2D-IDAPP meeting Valeria Di Felice University of Rome Tor Vergata Tutor: Prof. Piergiorgio Picozza Ferrara, 3-4 May 2007."— Presentation transcript:

1 2D-IDAPP meeting Valeria Di Felice University of Rome Tor Vergata Tutor: Prof. Piergiorgio Picozza Ferrara, 3-4 May 2007

2 Till now … Simulation Geometrical factor Jovian electrons Data Trapped particles Solar flares (COSPAR2006) PAMELA Collaboration Ferrara, 3-4 May 2007

3 Jovian electrons Periodicity: 1) 13 months (synodic year) 2) 27 days (CIRs modulation) Potgieter, M. S., Ferreira M, S. E. S.,J. Geophys. Res., 107, A7, 2002

4 Ferrara, 3-4 May 2007 Trapped particles 36 MeV p, 3.5 MeV e-

5 Ferrara, 3-4 May 2007 Flares S1 S2

6 Ferrara, 3-4 May 2007 Flares

7 Ferrara, 3-4 May 2007 In the future… Large amount of data => Analysis ! Going further (respect to the Solar System): looking for signals of exotic relevance (positrons, antiprotons spectra) ISAPP 2007 summer school Other … Thanks!

8 Ferrara, 3-4 May 2007 Flares Proton and Helium Selection Using tracker dedx

9 Ferrara, 3-4 May 2007 Flares

10 Ferrara, 3-4 May 2007 Flares

11 Ferrara, 3-4 May 2007 Flares

Download ppt "2D-IDAPP meeting Valeria Di Felice University of Rome Tor Vergata Tutor: Prof. Piergiorgio Picozza Ferrara, 3-4 May 2007."

Similar presentations

1 Introduction to the Standard Model Quarks and leptons Bosons and forces The Higgs Bill Murray, RAL, March 2002.

1 Introduction to the Standard Model Quarks and leptons Bosons and forces The Higgs Bill Murray, RAL, March 2002.
Light-nuclei discrimination of the space telescope PAMELA Roberta Sparvoli for the PAMELA Collaboration University of Rome Tor Vergata and INFN Rome (Italy)

Light-nuclei discrimination of the space telescope PAMELA Roberta Sparvoli for the PAMELA Collaboration University of Rome Tor Vergata and INFN Rome (Italy)
- DNA. Simulation of Interactions of Radiation with Biological Systems at the Cellular and DNA Level Based on Sponsored by Activity of S. Agostinelli,

- DNA. Simulation of Interactions of Radiation with Biological Systems at the Cellular and DNA Level Based on Sponsored by Activity of S. Agostinelli,
E. Mocchiutti, INFN Trieste - CALOR06 - 6 th June 2006, Chicago E. Mocchiutti 1, M. Albi 1, M. Boezio 1, V. Bonvicini 1, J. Lund 2, J. Lundquist 1, M.

E. Mocchiutti, INFN Trieste - CALOR th June 2006, Chicago E. Mocchiutti 1, M. Albi 1, M. Boezio 1, V. Bonvicini 1, J. Lund 2, J. Lundquist 1, M.
Implication of recent cosmic ray data Qiang Yuan Institute of High Energy Physics Collaborated with Xiaojun Bi, Hong Li, Jie Liu, Bing Zhang & Xinmin Zhang.

Implication of recent cosmic ray data Qiang Yuan Institute of High Energy Physics Collaborated with Xiaojun Bi, Hong Li, Jie Liu, Bing Zhang & Xinmin Zhang.
21 ECRS, Kosice, 12/09/2008 Trapped charge particles measurements in the radiation belt by PAMELA instrument Vladimir V. Mikhailov (MEPHI) for PAMELA collaboration.

21 ECRS, Kosice, 12/09/2008 Trapped charge particles measurements in the radiation belt by PAMELA instrument Vladimir V. Mikhailov (MEPHI) for PAMELA collaboration.
ROBERTA SPARVOLI UNIVERSITY OF ROME TOR VERGATA & INFN (ITALIAN NATIONAL INSTITUTE OF NUCLEAR PHYSICS) Results from the PAMELA space experiment.

ROBERTA SPARVOLI UNIVERSITY OF ROME TOR VERGATA & INFN (ITALIAN NATIONAL INSTITUTE OF NUCLEAR PHYSICS) Results from the PAMELA space experiment.
PAMELA Payload for Antimatter Matter Exploration and Light Nuclei Astrophysics.

PAMELA Payload for Antimatter Matter Exploration and Light Nuclei Astrophysics.
Numbers. 1 2 3 4 5 6 7 8 9 10 11 12 13.

Numbers
The ALTEA and ALTEA-Shield experiments onboard the International Space Station L. Di Fino, M. Larosa, L. Narici, V. Zaconte University of Rome Tor Vergata.

The ALTEA and ALTEA-Shield experiments onboard the International Space Station L. Di Fino, M. Larosa, L. Narici, V. Zaconte University of Rome Tor Vergata.
Results from PAMELA Mirko Boezio INFN Trieste, Italy On behalf of the PAMELA collaboration Indirect and Direct Detection of Dark Matter February 7 th 2011.

Results from PAMELA Mirko Boezio INFN Trieste, Italy On behalf of the PAMELA collaboration Indirect and Direct Detection of Dark Matter February 7 th 2011.
Solar Modulation: A Theoretical Perspective Modeling of cosmic ray charge-sign dependence in the heliosphere Marius Potgieter Unit for Space Physics North-West.

Solar Modulation: A Theoretical Perspective Modeling of cosmic ray charge-sign dependence in the heliosphere Marius Potgieter Unit for Space Physics North-West.
11 February 2000Genova (I)1 ESA Space Environment & Effects Analysis Section Space Radiation Environment P. Nieminen, ESA/ESTEC, The Netherlands  Overview.

11 February 2000Genova (I)1 ESA Space Environment & Effects Analysis Section Space Radiation Environment P. Nieminen, ESA/ESTEC, The Netherlands  Overview.
U NDERSTANDING C OSMIC R AYS AND S EARCHING FOR D ARK M ATTER WITH PAMELA Roberta Sparvoli for the PAMELA Collaboration University of Rome Tor Vergata.

U NDERSTANDING C OSMIC R AYS AND S EARCHING FOR D ARK M ATTER WITH PAMELA Roberta Sparvoli for the PAMELA Collaboration University of Rome Tor Vergata.
REMSIM Radiation Exposure and Mission Strategies for Interplanetary Manned Missions Susanna Guatelli, 9 th March 2004, Genova, Italy www.ge.infn.it/geant4/space/remsim.

REMSIM Radiation Exposure and Mission Strategies for Interplanetary Manned Missions Susanna Guatelli, 9 th March 2004, Genova, Italy
R. Sparvoli – MAPS 2009 - Perugia Outline of the lecture Lecture 2: Sources of background and their rejection Efficiencies & Contaminations Absolute fluxes.

R. Sparvoli – MAPS Perugia Outline of the lecture Lecture 2: Sources of background and their rejection Efficiencies & Contaminations Absolute fluxes.
 Production at forward Rapidity in d+Au Collisions at 200 GeV The STAR Forward TPCs Lambda Reconstruction Lambda Spectra & Yields Centrality Dependence.

 Production at forward Rapidity in d+Au Collisions at 200 GeV The STAR Forward TPCs Lambda Reconstruction Lambda Spectra & Yields Centrality Dependence.
Measurements of Cosmic-Ray Positrons & Electrons An Experimentalist’s Point of View Michael Schubnell University of Michigan February 4 th, 2009 XLIVth.

Measurements of Cosmic-Ray Positrons & Electrons An Experimentalist’s Point of View Michael Schubnell University of Michigan February 4 th, 2009 XLIVth.
Roberta Sparvoli University of Rome “Tor Vergata” and INFN Rome, Italy

Roberta Sparvoli University of Rome “Tor Vergata” and INFN Rome, Italy
U NDERSTANDING C OSMIC R AYS AND S EARCHING FOR D ARK M ATTER WITH PAMELA Roberta Sparvoli for the PAMELA Collaboration University of Rome Tor Vergata.

U NDERSTANDING C OSMIC R AYS AND S EARCHING FOR D ARK M ATTER WITH PAMELA Roberta Sparvoli for the PAMELA Collaboration University of Rome Tor Vergata.

Similar presentations

Ads by Google