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

Slides:



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

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,
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.
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.
PAMELA Payload for Antimatter Matter Exploration and Light Nuclei Astrophysics.
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.
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.
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.
REMSIM Radiation Exposure and Mission Strategies for Interplanetary Manned Missions Susanna Guatelli, 9 th March 2004, Genova, Italy
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.
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
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.
PAMELA SPACE MISSION ICHEP 2006 MOSCOW Piergiorgio Picozza Pamela collaboration INFN & University of Roma “Tor Vergata”
ROBERTA SPARVOLI UNIVERSITY OF ROME TOR VERGATA & INFN (ITALIAN NATIONAL INSTITUTE OF NUCLEAR PHYSICS) Recent results from the space experiment PAMELA.
1 PEBS Prototype PERDaix was launched in October 2010 from Kiruna, Sweden.
Roberta Sparvoli Roberta Sparvoli for the PAMELA Collaboration University of Rome Tor Vergata and INFN Roma II, Italy Uuuuuu Uuuu uuuuuuu.
The PAMELA Experiment: Preliminary Results after Two Years of Data Taking Emiliano Mocchiutti - INFN Trieste on behalf of the PAMELA Collaboration.
Antimatter What is Antimatter?  You cannot define antimatter without the speaking of matter.  Antimatter is equal and opposite to matter.  Since the.
Vladimir Mikhailov (NRNU MEPHI, Moscow) On behavior PAMELA collaboration SUB CUTOFF SPECTRA OF ELECTRONS AND POSITRONS measured in the PAMELA experiment.
The Alpha Magnetic Spectrometer (AMS) on the International Space Station (ISS) Maria Ionica I.N.F.N. Perugia International School.
Cosmic Ray Study The PAMELA Experiment Piergiorgio Picozza INFN and University of Rome Tor Vergata 23 rd European Cosmic Ray Symposium Moscow, Russia July.
H, He, Li and Be Isotopes in the PAMELA-Experiment Wolfgang Menn University of Siegen On behalf of the PAMELA collaboration International Conference on.
The method of the low-energy antiproton identification by stopping in the coordinate- sensitive PAMELA calorimeter 1 Svetlana Rodenko (MEPhI) Moscow International.
PAMELA measurements of proton and helium nuclei and cosmic ray acceleration in the galaxy M. Casolino RIKEN – ASI INFN & University of Rome Tor Vergata.
Simulation of Interactions of Radiation with Biological Systems at the Cellular and DNA Level Based on Sponsored by Activity of.
Propagation of CR electrons and the interpretation of diffuse  rays Andy Strong MPE, Garching GLAST Workshop, Rome, 17 Sept 2003 with Igor Moskalenko.
1. 2 ISS-present status Trent Martin NASA AMS Project Manager.
Capabilities of the Space Instrument PAMELA for Solar Research Roberta Sparvoli ON BEHALF OF THE PAMELA COLLABORATION University of Rome ‘‘Tor Vergata’’,
Direct measurements of cosmic rays in space ROBERTA SPARVOLI ROME “TOR VERGATA” UNIVERSITY AND INFN, ITALY Vulcano Workshop 2014 Vulcano Island (Italy),
Cultural Heritage and Sustainable Development E-Learning Program Second Videoconference Prof. P.L. Scandizzo University of Rome “Tor Vergata”
Electrostatic fluctuations at short scales in the solar-wind turbulent cascade. Francesco Valentini Dipartimento di Fisica and CNISM, Università della.
Measurements of cosmic ray particles in the energy range of – eV in the PAMELA experiment 21 st European Cosmic Ray Symposium, Ko š ice, Slovakia.
RIM Russian Italian Missions Piergiorgio Picozza INFN and University of “Rome Tor Vergata”
© OCR The periodic table is an essential tool for all chemists. It is full of useful information. RELATIVE ATOMIC MASS ATOMIC NUMBER SYMBOL helium.
Texting101 What words/phrases to the abbreviations in the text conversation represent? What are some other of abbreviations you use? Why do you think.
Antiproton and Electron Measurements and Dark Matter Searches
Roberta Sparvoli University of Rome ”Tor Vergata” and INFN
Internationalization
Mass of constituent parts of the nucleus:
The PAMELA Experiment: a Cosmic-Ray Experiment Deep Inside the Heliosphere Mirko Boezio INFN Trieste, Italy On behalf of the PAMELA collaboration ICRC.
Solar modulation of cosmic ray positrons in a quiet heliosphere
The Transition Radiation Detector for the PAMELA Experiment
Understanding CRs with Space Experiments
The High Energy Particle Detector for CSES Mission The Scientific Case
INFN & University of Roma “Tor Vergata”
INFN e Università di Roma Tor Vergata
Texting101 What words/phrases to the abbreviations in the text conversation represent? What are some other of abbreviations you use? Why do you think.
Imaging Dark Matter with the Pamela Experiment
L. Di Fino, M. Larosa, L. Narici, V. Zaconte
Roberta Sparvoli University of Rome ”Tor Vergata” and INFN
The magnetic spectrometer of PAMELA
Secondary positrons and electrons measured by PAMELA experiment
Vladimir Mikhailov (MEPhI) on behalf PAMELA collaboration
for the PAMELA collaboration
Physics: Concepts and Connections, 4th ed
Results from the PAMELA space experiment
Nicolo’ Masi, Andrea Tiseni TOF Group Bologna
What is the smallest particle of matter?
Habitable zones – where the incident flux from the star has a certain range of values, allowing liquid water to exist on a planet. If the flux we get from.
Picture 1 10 protons 10 neutrons = an electron.
The magnetic spectrometer of PAMELA
Presentation transcript:

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

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

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

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

Ferrara, 3-4 May 2007 Flares S1 S2

Ferrara, 3-4 May 2007 Flares

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!

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

Ferrara, 3-4 May 2007 Flares

Ferrara, 3-4 May 2007 Flares

Ferrara, 3-4 May 2007 Flares

Feedback: Privacy Policy Feedback
Do Not Sell My Personal Information
About project: SlidePlayer Terms of Service

© 2025 SlidePlayer.com. Inc. All rights reserved.