Cosmic ray transparency for a medium latitude observatory

Details Cosmic ray transparency for a medium latitude observatory Cosmic ray transparency for a medium latitude observatory

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ncimc..26..177b&link_type=abstract

Il Nuovo Cimento C, vol. 026, Issue 02, p.177

Physics

4

Scientific paper

The access of cosmic-ray particles to a medium-latitude observatory is analysed from results coming from the numerical solution of the charged-particle motion in the geomagnetic field. Evaluations are performed mainly for the Lomnický Štıt neutron monitor location (LS: 2634 m a.s.l., geographic coordinates 49.20° N, 20.22° E), but some results for the Antarctic Laboratory for Cosmic Rays (LARC: 40 m a.s.l, 62.20° S and 301.04° E) are also given. Particular attention is paid to the variability of the magnetospheric screening appearing when the external magnetic field is added to the internal one.

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