International School of Cosmic Ray Astrophysics

16th  Course: "Gamma Ray and Cosmic Ray Astrophysics: From below GeV to beyond EeV Energies"

 5-12 July 2008
Ettore Majorana Centre
Erice, Sicily, Italy

 

Presenter

Titles/Presentations

Marco Casolino (CV)
  Universita di Roma
  Rome, Italy

(1) PAMELA (Part 1)  (Part 2)
(2)
Study of cosmic rays of galactic, solar, terrestrial and unknown origin with Pamela detector: first results.

Martin Israel (CV)
  Washington University
  St. Louis, Mo. USA
(1) What we Learn from Observation of Cosmic Ray Isotopic Composition
(2)
Evidence for Cosmic Ray Origin in Galactic OB Associations
Leonidas Resvanis (CV)
  University of Athens
  Athens, Greece
(1) Neutrino Astronomy and High Energy Neutrino Telescopes (Part 1) (Part 2)
Vladimir Ptuskin (CV)
  IZMIRAN, RAS
  Troitsk, Russia
(1) Diffusive Shock Acceleration
(2) Supernova remnants as particle Accelerators

Todor Stanev (CV)
  Bartol Research Institute
  Bartol, DL, USA

(1) Propagation of Ultrahigh Energy Cosmic Rays in the Universe.
(2) Neutrino Oscillations
(3) Search for High Energy Neutrinos with Detectors Deployed in Antarctic Ice.

Marco Tavani
  IASF/INAF Roma
  Rome, Italy
(1) Gamma Ray Astrophysics with AGILE

Masahiro Teshima (CV)
  Max Plank Institute
  Munich, Germany

(1) CTA; Next Generation Ground-Based Gamma-Ray Observatory
(2) Highlights of High Energy Gamma Ray Astronomy

Alan Watson (CV)
  University of Leeds
  Leeds, UK.

(1) The Physics of Extensive Air Showers and the Pierre Auger Observatory
(2) First results from the Pierre Auger Observatory - the birth of the hybrid era.

John Wefel (CV)
  Louisiana State University
  Baton Rouge, LA, USA
(1) Cosmic Ray Electrons
(2) The Emergence of Particle Astrophysics in the Space Age

Gaurang Yodh (CV)
  University of California
  Irvine, Ca, USA

(1) TeV Gamma Ray Astronomy with Air Shower Telescopes
(2) Cosmic Rays from the Knee to the Ankle
Shigehiro Nagataki (CV)
  Kyoto University
  Kyoto, Japan
(1) High Energy Neutrino Astronomy
Thomas Hams (CV)
  CRESST/USRA
  Greenbelt, MD USA
(1) BESS-Polar Program and the Search for Antimatter

Participant Presentations

Presenter

Titles/Presentations

Terri Brandt
  Ohio State University
  Columbus, Oh USA
Overview of the CREAM Experiment and the Flight of CREAM III
Rogerio Menezes de Almeida
  UNICAMP
  Campinas, Brazil
Search for UHECRs from SGR1806-20 with Pierre Auger Observatory
Jairo Cavalcante de Souza
  University of Sao Paulo
  San Paulo, Brazil
Searching for Supersymmetry through UHECR
Kamlesh Dookayka
  University of California
  Irvine, CA USA
Simulating Surface Roughness and its effects on EM wave scattering for ANITA
Gema Hebrero
  Universidad de Alcala
  Madrid, Spain
Behavior of Iron Charge States in Solar Flares produced in the Solar Corona Plasma: Results of Escape Model
Paula Gina Isar
  Forschungszentrum
  Karlsruhe, Germany
Radio Detection of Cosmic Ray Air Showers with LOPES
 Juan Cruz Moreno
  Instituto de Fisica
  La Plata, Argentina
Atmospheric Depth Profile: A New Model for an Old Subject
Andreas Obermeier
  University of Chicago
  Chicago, Il USA
Galactic Propagations and Source Abundances of Cosmic Ray Nuclei at High Energies
Roberto Lineros Rodriguez
  Universita di Torino
  Torino, Italy
Positrons from Dark Matter Annihilation in the Galactic Halo: Theoretical Uncertainties
Iurii Sushch
  Nat'l Taras Shevchenko University
  Kyiv, Ukraine
VELA Supernova Remnant Evolution in the Inhomogeneous Interstellar Medium
Hajame Takami
  University of Tokyo
  Tokyo, Japan
Cross Correlation Study between UHECR Arrival Distribution and Nearby Large-scale Structure
Stephanie Wissel
  University of Chicago
  Chicago, IL USA
Direct Cherenkov Method of detecting VHE Cosmic Rays with Ground Based Detectors.

 

30 Years of Maury Shapiro's ISCRA

Presenter

Titles/Presentations

John Wefel
   LSU
(1) Retrospective on 30 years of the ISCRA
(2) ISCRA-2010
Susan Ames
   Oxford
(1)  Propagating Cosmic Rays with Maury
Gaurang Yodh
   UC-Irvine
(1) Early Years working with Maury
Arthur Smith
   Oxford
(1) A Recollection of Professor Shapiro

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