Evolution of the cosmic ray spectrum during a Forbush decrease-Reference-Cited by-同舟云学术

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Evolution of the cosmic ray spectrum during a Forbush decrease

Published:2024-05 Issue:9 Volume:73 Page:4842-4852
ISSN:0273-1177
Container-title:Advances in Space Research
language:en
Short-container-title:Advances in Space Research

Author:

Blanco Juan José,Ayuso Sindulfo,Regadío Alberto,López-Comazzi Alejandro,García-Tejedor Juan Ignacio,García-Población Óscar,Guerrero Contreras Carlo Luis

Funder

Ministerio de Ciencia e Innovación

España Ministerio de Ciencia e Innovación

Publisher

Elsevier BV

Reference33 articles.

1. Mito: a new directional muon telescope;Ayuso;J. Space Weather Space Clim.,2021

2. The Large-Scale Magnetic Field Configuration Associated With Forbush Decreases;Barnden,1973

3. What determines the magnitude of forbush decreases?;Belov;Adv. Space Res.,2001

4. On the rigidity spectrum of cosmic-ray variations within propagating interplanetary disturbances: Neutron monitor and soho/ephin observations at 1–10 gv;Belov;Astrophys. J.,2021

5. Observable Effects of Interplanetary Coronal Mass Ejections on Ground Level Neutron Monitor Count Rates;Blanco;Solar Physics,2013

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