Abstract
The experimental values of the geomagnetic cosmic-ray effects have been used in calculating the change of cosmic-ray intensity during a magnetic storm on the assumption that the magnetic disturbance can be regarded as a variation of the Earth's magnetic moment. The change in moment found necessary to produce the observed variations of cosmic-ray intensity during the storm of April 1937 is of the order 150 times greater than any value simply reconcilable with the magnetic disturbances recorded.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
