Abstract
The different types of cosmic ray intensity variations arising from the semidiurnal anisotropy are evaluated for different stations taking into consideration the effect of the Earth's axis inclination. Appropriate values of the parameters of the anisotropy together with accurate values of coupling and normalization constants are used in the calculations. The results predict the appearance of semiannual and diurnal waves as a consequence of a semidiurnal anisotropy. The form of the generated waves are found to be dependent on the characteristics of the station's asymptotic cone of acceptance as well as the season of detection. The characteristics of these waves together with that of the semidiurnal variation are discussed in detail.
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.
