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