Measurement and simulation of neutron monitor count rate dependence on surrounding structure-Reference-Cited by-同舟云学术

Measurement and simulation of neutron monitor count rate dependence on surrounding structure

Published:2015-07 Issue:7 Volume:120 Page:5253-5265
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Aiemsa‐ad N.¹²³,Ruffolo D.³⁴^ORCID,Sáiz A.³⁴,Mangeard P.‐S.⁴⁵,Nutaro T.³⁶,Nuntiyakul W.³⁴⁷,Kamyan N.⁴,Khumlumlert T.¹,Krüger H.⁸,Moraal H.⁸,Bieber J. W.⁹,Clem J.⁹,Evenson P.⁹

Affiliation:

1. Department of Physics, Faculty of Science Naresuan University Phitsanulok Thailand

2. Faculty of Science and Technology Rajabhat Rajanagarindra University Chachoengsao Thailand

3. Thailand Center of Excellence in Physics CHE, Ministry of Education Bangkok Thailand

4. Department of Physics, Faculty of Science Mahidol University Bangkok Thailand

5. National Astronomical Research Institute of Thailand Chiang Mai Thailand

6. Department of Physics, Faculty of Science Ubon Ratchathani University Ubon Ratchathani Thailand

7. Faculty of Science Chandrakasem Rajabhat University Bangkok Thailand

8. Centre for Space Research, School of Physical and Chemical Sciences North‐West University Potchefstroom South Africa

9. Bartol Research Institute, Department of Physics and Astronomy University of Delaware Newark Delaware USA

Funder

National Science Foundation

Thailand Research Fund

Mahidol University

South African National Science Foundation

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/2015JA021249

Reference31 articles.

1. TIME DEPENDENCE OF THE PROTON FLUX MEASURED BY PAMELA DURING THE 2006 JULY-2009 DECEMBER SOLAR MINIMUM

2. Impact of atmospheric parameters on the atmospheric Cherenkov technique

3. Latitude survey observations of neutron monitor multiplicity

4. The FLUKA Code: Developments and Challenges for High Energy and Medical Applications

5. Cosmic-ray yield and response functions in the atmosphere

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