Atmospheric Secondary Charged Cosmic Radiation at a place of 11.5 GV Geomagnetic Cut-Off

Details Atmospheric Secondary Charged Cosmic Radiation at a place of 11.5 GV Geomagnetic Cut-Off Atmospheric Secondary Charged Cosmic Radiation at a place of 11.5 GV Geomagnetic Cut-Off

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006head....9.1866a&link_type=abstract

American Astronomical Society, HEAD meeting #9, #18.66; Bulletin of the American Astronomical Society, Vol. 38, p.393

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An experiment performed with a balloon-borne plastic scintillator is described. The detector system was transported by a stratospheric balloon, that was launched from a place with a geomagnetic cut-off of 11.5 GV, from Argentina, on 27 May 1998. Spectra for both the charged component of the secondary cosmic radiation and the atmospheric gamma-radiation were alternatively measured at different altitudes, during the ascent of the balloon, and at ceiling altitude. The atmospheric gamma radiation was analyzed elsewhere. The energy loss spectrum is explained , at least qualitatively, by the computation of the response of the detector to charged radiation. This research was supported by CONICET, from Argentina.

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