Inelastic Proton-Air Cross Section Growth From 0.2 TeV to 10 PeV According to TIEN SHAN Experimental Cosmic Ray Data

EPJ Web of Conferences - France
doi 10.1051/epjconf/201714519001
Full Text
Abstract

Available in full text

Date
Authors
Publisher

EDP Sciences

Related search

Extrapolation of Proton-Proton Cross Section to Cosmic Ray Energies Using Geometrical Model

EPJ Web of Conferences
AstronomyPhysics
2017English

Modern Status of the Tien-Shan Cosmic Ray Station

EPJ Web of Conferences
AstronomyPhysics
2017English

Three Component Model of Cosmic Ray Spectra From 10 GeV to 100 PeV

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2006English

TeV-PeV Neutrino-Nucleon Cross Section Measurement With 5 Years of IceCube Data

2018English

Measurement of the Cosmic Ray Proton Spectrum From 40 GeV to 100 TeV With the DAMPE Satellite

Science advances
Multidisciplinary
2019English

Hardening Effects of the TeV-scale Cosmic Ray Proton and Helium Spectra

2019English

Extrapolation of Nucleus-Nucleus Cross Section to Cosmic Ray Energies Using Geometrical Model

2017English

Estimation of Slip Rates in the Southern Tien Shan Using Cosmic Ray Exposure Dates of Abandoned Alluvial Fans

Bulletin of the Geological Society of America
Geology
1998English

Data-Driven Model of the Cosmic-Ray Flux and Mass Composition From 10 GeV to $10^{11}$ GeV

2017English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2025 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy