Can we properly model the neutron monitor count rate?-Reference-Cited by-同舟云学术

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Can we properly model the neutron monitor count rate?

Published:2015-09 Issue:9 Volume:120 Page:7172-7178
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Gil Agnieszka¹²,Usoskin Ilya G.²³,Kovaltsov Gennady A.⁴,Mishev Alexander L.²,Corti Claudio⁵,Bindi Veronica⁵

Affiliation:

1. Institute of Mathematics and PhysicsSiedlce University Siedlce Poland

2. ReSoLVE Centre of ExcellenceUniversity of Oulu Oulu Finland

3. Sodankylä Geophysical ObservatoryUniversity of Oulu Oulu Finland

4. Ioffe Physical‐Technical Institute St. Petersburg Russia

5. Department of Physics and Astronomy University of Hawai‘i at Mānoa Honolulu Hawaii USA

Funder

Foundation for Polish Science (A.G)

ReSoLVE Centre of Excellence (Academy of Finland)

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/2015JA021654

Reference37 articles.

1. Efficiency of detection for neutron detectors with different geometries

2. PAMELA Measurements of Cosmic-Ray Proton and Helium Spectra

3. The PAMELA Mission: Heralding a new era in precision cosmic ray physics

4. First Result from the Alpha Magnetic Spectrometer on the International Space Station: Precision Measurement of the Positron Fraction in Primary Cosmic Rays of 0.5–350 GeV

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