Research on Cosmic Rays and Their Impact on Human Activities

The galactic cosmic–ray spectrum extends over 14 orders of magnitudes in energy and about 12 orders of magnitude in intensity, and it can be studied using two different methods: via the “direct detection” of the primary cosmic rays in space or at high altitude and via the “indirect detection” of sec...

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Year of Publication:2022
Language:English
Physical Description:1 electronic resource (140 p.)
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520 |a The galactic cosmic–ray spectrum extends over 14 orders of magnitudes in energy and about 12 orders of magnitude in intensity, and it can be studied using two different methods: via the “direct detection” of the primary cosmic rays in space or at high altitude and via the “indirect detection” of secondary particles, namely the extensive air showers produced by a primary cosmic–ray particle impinging the atmosphere. In this Special Issue, both direct and indirect measurements are presented via from various experiments. Emphasis is placed on low-energy electrons and protons that are detected in flight as well as during geomagnetic storms. As for indirect detection, the muon flux determination and modulation at ground level are described in great detail. Some of the most interesting results are hereby presented, and a couple of new techniques in cosmic–ray detection are reported. 
546 |a English 
650 7 |a Research & information: general  |2 bicssc 
650 7 |a Mathematics & science  |2 bicssc 
653 |a cosmic rays 
653 |a Extensive Air Showers 
653 |a particle detectors 
653 |a Cosmic Ray Ensembles 
653 |a ionosphere 
653 |a ELF/VLF waves 
653 |a energetic electron precipitations 
653 |a storm-time feature 
653 |a CSES 
653 |a trapped particles 
653 |a South Atlantic Anomaly 
653 |a AE9/AP9/SPM models 
653 |a radiation belts 
653 |a Poisson data 
653 |a time series 
653 |a quasi-Gaussian filter 
653 |a digital filtering 
653 |a optimization 
653 |a global minimization 
653 |a annealing simulation algorithm 
653 |a space weather 
653 |a geomagnetic storms 
653 |a LEO satellites 
653 |a digital gamma-rays spectrometer 
653 |a cosmic veto 
653 |a active shield 
653 |a muons 
653 |a muon flux periodicity 
653 |a atmospheric neutrons 
653 |a radiation dose 
653 |a passengers and flight crew 
653 |a ultrathin calorimeter 
653 |a direct measurements 
653 |a energy reconstruction 
653 |a PAMELA 
653 |a shower development universality 
653 |a cosmic ray physics 
653 |a multi-messenger astrophysics 
653 |a extensive air showers 
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