| タイトル | The structure of EAS at E 0.1 EeV |
| 本文（外部サイト） | http://hdl.handle.net/2060/19850027699 |
| 著者（英） | Loh, E. C.; Steck, D.; Gerhardy, P. R.; Sokolsky, P.; Elbert, J. W.; Cooper, R.; Baltrusaitis, R. M.; Mizumoto, Y.; Cassiday, G. L. |
| 著者所属（英） | Utah Univ. |
| 発行日 | 1985-08-01 |
| 言語 | eng |
| 内容記述 | The ratio of extensive air showers (EAS) total shower energy in the electromagnetic channel (E em) to the size of the shower at maximum development (N max) from a direct measurement of shower longitudinal development using the air fluorescence technique was calculated. The values are not inconsistent with values based upon track length integrals of the Gaisser-Hillas formula for shower development or the known relation between shower energy and size at maximum for pure electromagnetic cascades. Using Linsley's estimates for undetected shower energy based on an analysis of a wide variety of cosmic ray data, the following relation for total shower energy E vs N max is obtained. The Gaisser Hillas implied undetected shower energy fractions. |
| NASA分類 | SPACE RADIATION |
| レポートNO | 85N36012
HE-4.4-2 |
| 権利 | No Copyright |
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