The Behaviour of Galactic Cosmic-Ray Intensity During Solar Activity Cycle 24. (2019)

First Author: Ross E

Attributed to: Helioseismology at Birmingham and Queen Mary funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1007/s11207-019-1397-7

PubMed Identifier: 30872867

Publication URI: http://europepmc.org/abstract/MED/30872867

Type: Journal Article/Review

Volume: 294

Parent Publication: Solar physics

Issue: 1

ISSN: 0038-0938