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

doi 10.22323/1.301.0533

Full Text

Abstract

Available in

Date

Authors

Publisher

Sissa Medialab

Related search

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

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2006English

Energy Spectrum of the Primary Cosmic Rays in the Range 10 GeV–10 TeV

2016English

An Interpretation of the Cosmic Ray E+ + E− Spectrum From 10 GeV to 3 TeV Measured by CALET on the ISS

International Journal of Modern Physics D
AstrophysicsAstronomyPlanetary ScienceMathematical PhysicsSpace
2019English

The Cosmic‐Ray Antiproton Flux Between 0.62 and 3.19 GeV Measured Near Solar Minimum Activity

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
1997English

Scaled Simulations of a 10 GeV Accelerator

2009English

Hadronic Physics With Electrons Beyond 10 GeV

Nuclear Physics A
High Energy PhysicsNuclear
1991English

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

Science advances
Multidisciplinary
2019English

Cosmic-Ray Electron-Positron Spectrum From 7 GeV to 2 TeV With the Fermi Large Area Telescope

Physical Review D
AstronomyPhysics
2017English

GeV-TeV Cosmic-Ray Spectral Anomaly as Due to Reacceleration by Weak Shocks in the Galaxy

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2014English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2026 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy