Abstract
An attempt is made to examine the energy gain or loss of the primary cosmic ray produced by an electro-magnetic field of solar stream, and then to explain the diurnal variation of cosmic rays at the time of the magnetic storm by this energy variation of cosmic rays.The amplitudes and the times of the maximum intensity of the diurnal variations are calculated at various altitudes and latitudes by using the above mentioned electric field.Whether the diurnal variation of cosmic rays averaged over all days can be explained or not from the standpoint of the electric field hypothesis is also discussed.
Sign-in/Register to access full text options 
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.
