The High Energy Cosmic Radiation Facility onboard China's Space Station

2016 ◽  
Vol 279-281 ◽  
pp. 161-165 ◽  
Author(s):  
M. Xu
Keyword(s):  
Cosmic Radiation ◽  
Space Station ◽  
High Energy

scholarly journals A novel 3-D calorimeter for the High Energy cosmic-Radiation Detection (HERD) Facility onboard China’s Future Space Station

2017 ◽  
Author(s):  
Yongwei Dong ◽  
Ming Xu ◽  
Zhigang Wang ◽  
Oscar Adriani ◽  
Sebastiano Albergo ◽  
...  
Keyword(s):  
Cosmic Radiation ◽  
Radiation Detection ◽  
Space Station ◽  
High Energy ◽  
Future Space

scholarly journals Introduction to the High Energy cosmic-Radiation Detection (HERD) Facility onboard China’s Future Space Station

2017 ◽  
Author(s):  
Shuang-Nan Zhang ◽  
Oscar Adriani ◽  
Herd Consortium ◽  
Sebastiano Albergo ◽  
Giovanni Ambrosi ◽  
...  
Keyword(s):  
Cosmic Radiation ◽  
Radiation Detection ◽  
Space Station ◽  
High Energy ◽  
Future Space

scholarly journals Perspective of monochromatic gamma-ray line detection with the High Energy cosmic-Radiation Detection (HERD) facility onboard China’s space station

2016 ◽  
Vol 78 ◽  
pp. 35-42 ◽  
Author(s):  
Xiaoyuan Huang ◽  
Anna S. Lamperstorfer ◽  
Yue-Lin Sming Tsai ◽  
Ming Xu ◽  
Qiang Yuan ◽  
...  
Keyword(s):  
Cosmic Radiation ◽  
Gamma Ray ◽  
Radiation Detection ◽  
Space Station ◽  
High Energy ◽  
Line Detection

scholarly journals The high energy cosmic-radiation detection (HERD) facility onboard China's Space Station

2014 ◽  
Author(s):  
S. N. Zhang ◽  
O. Adriani ◽  
S. Albergo ◽  
G. Ambrosi ◽  
Q. An ◽  
...  
Keyword(s):  
Cosmic Radiation ◽  
Radiation Detection ◽  
Space Station ◽  
High Energy

scholarly journals Properties of Elementary Particle Fluxes in Primary Cosmic Rays Measured with the Alpha Magnetic Spectrometer on the International Space Station

2019 ◽  
Vol 209 ◽  
pp. 01007
Author(s):  
Francesco Nozzoli
Keyword(s):  
Electron Flux ◽  
Space Station ◽  
Cosmic Ray ◽  
High Energy ◽  
Precision Measurements ◽  
High Energy Electrons ◽  
Electrons And Positrons ◽  
Positron Flux ◽  
Rigidity Dependence ◽  
Alpha Magnetic Spectrometer

Precision measurements by AMS of the fluxes of cosmic ray positrons, electrons, antiprotons, protons as well as their rations reveal several unexpected and intriguing features. The presented measurements extend the energy range of the previous observations with much increased precision. The new results show that the behavior of positron flux at around 300 GeV is consistent with a new source that produce equal amount of high energy electrons and positrons. In addition, in the absolute rigidity range 60–500 GV, the antiproton, proton, and positron fluxes are found to have nearly identical rigidity dependence and the electron flux exhibits different rigidity dependence.

The HERO project for the study of high-energy primary cosmic radiation

2009 ◽  
Vol 73 (5) ◽  
pp. 593-596
Author(s):  
D. M. Podorozhnyi ◽  
E. V. Atkin ◽  
L. S. Burylov ◽  
A. G. Voronin ◽  
N. V. Kuznetsov ◽  
...  
Keyword(s):  
Cosmic Radiation ◽  
High Energy ◽  
Primary Cosmic Radiation

Detectors for cosmic particles, neutrinos and exotic matter

2020 ◽  
pp. 655-710
Author(s):  
Hermann Kolanoski ◽  
Norbert Wermes
Keyword(s):  
Dark Matter ◽  
Particle Physics ◽  
Cosmic Radiation ◽  
Charged Particles ◽  
Cosmic Ray ◽  
High Energy ◽  
Detection Methods ◽  
Astroparticle Physics ◽  
High Energy Cosmic Rays ◽  
Cosmic Origin

Astroparticle physics deals with the investigation of cosmic radiation using similar detection methods as in particle physics, however, mostly with quite different detector arrangements. In this chapter the detection principles for the different radiation types with cosmic origin are presented, this includes charged particles, gamma radiation, neutrinos and possibly existing Dark Matter. In the case of neutrinos also experiments at accelerators and reactors are included. Examples, which are typical for the different areas, are given for detectors and their properties. For cosmic ray detection apparatuses are deployed above the atmosphere with balloons or satellites or on the ground using the atmosphere as calorimeter in which high-energy cosmic rays develop showers or in underground areas including in water and ice.

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