Physics
Scientific paper
Jul 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....1..203i&link_type=abstract
Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I
Physics
Scientific paper
The cosmic ray (CR) intensity variations are observed by using indep endent sets of compact extensive air shower (EAS) arrays. The Large Area Air Shower (LAAS) group deploys 9 EAS arrays in hundreds of km baseline scattered over a large part of Japan. The barometric coefficients for EAS counting rates are determined for each array. The atmospheric dynamics becomes the sub ject by using CR intensity tomography. The cross-correlation functions between intensity data observed at each array are examined to determine both time and spatial scales of atmospheric structures. The barometric coefficients of EAS intensity are about -0.6%/hPa for all arrays, and the cross-correlations in EAS data between arrays are observed and their amplitudes are larger than that of barometric pressure data.
Fujiwara Yasuhiro
Iyono Atsushi
Konishi Tetsuro
LAAS Group
Nakamura Takashi
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