Abstract
29182 stars observed at mountain altitudes in Kenya are analysed statistically. The analysis gives: — (1) An absorption thickness of 149 g/cm2 near the geomagnetic equator. (2) The star frequency as a function of the total number of prongs in a star is the result of the composition of the emulsion. (3) The empirical formula of Teucher for the energy of the star producing particle can be used in our experiments. (4) The variation in the number of shower particles with the complexity of the star and the altitude appears to be in agreement with the Heisenberg theory of the plural production of mesons.
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.
