3-11 July 2007
Merida, Mexico
Mexico/General timezone
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OG 1.5

Place

Location: Merida, Mexico
Room: Kabah (Holiday Inn)
Date: 6 Jul 10:30 - 11:55

Timetable | Contribution List

Displaying 7 contributions out of 7
Type: Oral Session: OG 1.5
Track: OG.1.5
We are proposing the CALET mission carried out on the Japanese Experiment Module of International Space Station. Major purpose of the mission is to search for the nearby cosmic ray sources and dark matter. The detector consists of an imaging calorimeter and a total absorption calorimeter to detect the electrons and the gamma-rays up to 10 TeV with very efficient rejection power of th ... More
Presented by Prof. Shoji TORII on 6/7/2007 at 16:06
Type: Oral Session: OG 1.5
Track: OG.1.5
The Cosmic Ray Energetics And Mass (CREAM) experiment has now flown over Antarctica for a total of 70 days, combining a record-breaking continuous 42 days in the air with a second Long Duration Balloon flight. The array of detection techniques utilized by CREAM includes a Timing Charge Detector, a Transition Radiation Detector, a Silicon Charge Detector, and a tracking Calorimeter to obtain th ... More
Presented by T. J. BRANDT on 6/7/2007 at 16:42
Type: Oral Session: OG 1.5
Track: OG.1.5
The PAMELA (Payload for Antimatter Matter Exploration and Light nuclei Astrophysics) experiment is a satellite-borne apparatus mounted on the Resurs DK1 russian satellite, launched from the Baikonur cosmodrome on June 15th 2006. It is designed to study charged particles in the cosmic radiation with a particular focus on antiparticles and light nuclei. The PAMELA apparatus comprises a time-o ... More
Presented by Dr. Giuseppe OSTERIA on 6/7/2007 at 16:30
Type: Oral Session: OG 1.5
Track: OG.1.5
The observation of a possible excess in the cosmic-ray positron spectrum has been suggested to originate from WIMP annihilations in the halo of the Galaxy. To measure this spectrum in the interesting energy range of 1-100 GeV with high precision, we are developing a dedicated balloon-borne spectrometer (PEBS). The best measurement of the cosmic-ray positron flux available today was perform ... More
Presented by Mr. Henning GAST on 6/7/2007 at 15:54
Type: Oral Session: OG 1.5
Track: OG.1.5
CREST is a balloon-borne detector array of barium fluoride crystal scintillators which will measure the intensity and spectrum of multi-TeV electrons in the Cosmic Rays. By detecting the synchrotron photons emitted from electrons passing through the earth's magnetic field, CREST's acceptance is several times its geometric area. We present background measurement results from a small arra ... More
Presented by Dr. Michael SCHUBNELL on 6/7/2007 at 15:30
Type: Oral Session: OG 1.5
Track: OG.1.5
Cosmic ray electrons with energies greater that about 300 GeV are of particular interest because, due to their high energy losses during interstellar propagation, there are likely to be only a small number of nearby sources contributing to the electron energy spectrum above several hundred GeV. It has been suggested that this may result in observable structure. Further, if the annihilation o ... More
Presented by Prof. T. Gregory GUZIK on 6/7/2007 at 15:42
Type: Oral Session: OG 1.5
Track: OG.1.5
The present status of the PAMELA electromagnetic calorimeter on board the satellite Resurs-DK1 will be presented. The PAMELA apparatus was put in orbit on 15 June 2006. The main task of the calorimeter is to select cosmic-ray antiprotons and positrons in a vast background of electrons and protons respectively with an high rejection power. Furthermore, the calorimeter is equipped with a s ... More
Presented by Dr. Emiliano MOCCHIUTTI on 6/7/2007 at 16:18
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