In this paper we present a Monte Carlo study of a calorimeter response for an experiment to equip the magnetic facility of the USA space station. Main purpose in the design of such a calorimeter is the efficient discrimination between eloctromagnetic and hadronic showers. The estimated rejection power results to be better than 1·10−3 p/e+ for incident particles with energy between 10 GeV and 100GeV
The best measurement of the cosmic ray positron flux available today was performed by the HEAT ballo...
AMS-02 (Alpha Magnetic Spectrometer) is a cosmic rays detector installed in May 2011 on the Internat...
The direct observation of high-energy cosmic rays, up to the PeV region, will depend on highly perfo...
An imaging calorimeter has been designed and is being built for the PAMELA satellite-borne experimen...
Abstract The silicon sampling calorimeter presented is conceived as a fine grained imaging device ...
The AMS-02 experiment is a particle detector installed on the International Space Station (ISS) sinc...
This paper describes the Monte Carlo program used for the simulation of antiproton interactions at i...
The WiZard Collaboration is involved in a program studying the antimatter components of the cosmic r...
A silicon-tungsten sampling imaging calorimeter has been designed and built for the PAMELA satellite...
Abstract: The 3D imaging calorimeter of AMS was designed to precisely reconstruct the longitudinal a...
In many physics experiments where calorimeters are employed, the requirement of an accurate energy m...
The High Energy cosmic-Radiation Detection (HERD) facility onboard China's Space Station is planned ...
Abstract This report presents the results obtained with a prototype silicon-tungsten (Si-W) electr...
Direct measurements of charged cosmic radiation with instruments in Low Earth Orbit (LEO), or flying...
The High Energy cosmic-Radiation Detection (HERD) facility onboard China’s Space Station is planned ...
The best measurement of the cosmic ray positron flux available today was performed by the HEAT ballo...
AMS-02 (Alpha Magnetic Spectrometer) is a cosmic rays detector installed in May 2011 on the Internat...
The direct observation of high-energy cosmic rays, up to the PeV region, will depend on highly perfo...
An imaging calorimeter has been designed and is being built for the PAMELA satellite-borne experimen...
Abstract The silicon sampling calorimeter presented is conceived as a fine grained imaging device ...
The AMS-02 experiment is a particle detector installed on the International Space Station (ISS) sinc...
This paper describes the Monte Carlo program used for the simulation of antiproton interactions at i...
The WiZard Collaboration is involved in a program studying the antimatter components of the cosmic r...
A silicon-tungsten sampling imaging calorimeter has been designed and built for the PAMELA satellite...
Abstract: The 3D imaging calorimeter of AMS was designed to precisely reconstruct the longitudinal a...
In many physics experiments where calorimeters are employed, the requirement of an accurate energy m...
The High Energy cosmic-Radiation Detection (HERD) facility onboard China's Space Station is planned ...
Abstract This report presents the results obtained with a prototype silicon-tungsten (Si-W) electr...
Direct measurements of charged cosmic radiation with instruments in Low Earth Orbit (LEO), or flying...
The High Energy cosmic-Radiation Detection (HERD) facility onboard China’s Space Station is planned ...
The best measurement of the cosmic ray positron flux available today was performed by the HEAT ballo...
AMS-02 (Alpha Magnetic Spectrometer) is a cosmic rays detector installed in May 2011 on the Internat...
The direct observation of high-energy cosmic rays, up to the PeV region, will depend on highly perfo...