The key observables of the KASCADE field array are the electron and muon number of extensive air showers. Using the size spectra of these measured quantities and their correlations with energy and primary mass it is possible to reconstruct the energy spectra of individual mass groups. The analysis
β¦ LIBER β¦
Regions of the maximal cosmic ray energy release in the atmosphere
β Scribed by A. V. Blinov; Yu. A. Kropotina
- Book ID
- 110163958
- Publisher
- SP MAIK Nauka/Interperiodica
- Year
- 2009
- Tongue
- English
- Weight
- 240 KB
- Volume
- 49
- Category
- Article
- ISSN
- 0016-7932
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