2005/06/28 by E. S. Nikiforova, Nikiforova, E. S.
Engineering · Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #Ranque-Hilsch vortex tube #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0506679
4 pages,4 figure, the paper will be published in Proc. 29th Int. Cosmic Ray Conf., Pune, India,2005
arxiv created 2005/06/28 · openalex publication_date 2005/06/28 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28
The dependence of the number of extensive air showers (EAS) on the zenith angle is obtained in groups with a constant solid-angle step with different election types at separations between stations of 500 and 1000 m by using the Yakutsk EAS array data. A bend point is formed at the zenith angle approximately of 50 deg. This point shifts with the increasing energy in the direction corresponding to the shift of the cascade-curve maximum depth with the variation of energy. The boundaries of change of these dependences obtained separately at the distances between stations of 500 and 1000 m are different that may be caused by the uncertainty of the lateral distribution function (LDF) used. Thereby, energies of showers detected by the stations with a different separation are not joined.