Evidence for changing of cosmic ray composition between 10(17) and 10(18) eV from multicomponent measurements

Update Item Information
Publication Type Journal Article
School or College College of Science
Department Physics
Creator Kieda, David B.
Other Author Abu-Zayyad, T.; Belov, K.; Bird, J.; Cao, Z.; Catanese, M.; Chen, G. F.; Clay, R. W.; Covault, C. E.; Cronin, J. W.; Dai, H. Y.; Dawson, B. R.; Elbert, J. W.; Fick, B. E.; Fortson, L. F.; Fowler, J. W.; Gibbs, K. G.; Glasmacher, M. A. K.; Green, K. D.; Ho, Y.; Huang, A.; Jui, C. C.; Kidd, M. J.; Knapp, B. C.; Ko, S.; Larsen, C. G.; Lee, W.; Loh, E. C.; Mannel, E. J.; Matthews, J.; Matthews, J. N.; Newport, B. J.; Nitz, D. F.; Ong, R. A.; Simpson, K. M.; Smith, J. D.; Sinclair, D.; Sokalsky, P.; Sommers, P.; Song, C.; Tang, J. K. K,; Thomas, S. B.; van der Velde, J. C.; Wiencke, L. R.; Wilkinson, C. R.; Yoshida, S.; Zhang, X. Z.
Title Evidence for changing of cosmic ray composition between 10(17) and 10(18) eV from multicomponent measurements
Date 2000
Description The average mass composition of cosmic rays with primary energies between 1017 and 1018 eV has been studied using a hybrid detector consisting of the High Resolution Fly's Eye (HiRes) prototype and the MIA muon array. Measurements have been made of the change in the depth of shower maximum and the muon density as a function of energy. The results show that the composition is changing from a heavy to lighter mix as the energy increases.
Type Text
Publisher American Physical Society
Volume 84
Issue 19
First Page 4276
Last Page 4279
Subject Cosmic rays; Particle energy; Muon array
Subject LCSH Cosmic rays; Muons; Particles
Language eng
Bibliographic Citation Abu-Zayyad, T., Belov, K., Bird, J., Cao, Z., Catanese, M., Chen, G. F., Clay, R. W., Covault, C. E., Cronin, J. W., Dai, H. Y., Dawson, B. R., Elbert, J. W., Fick, B. E., Fortson, L. F., Fowler, J. W., Gibbs, K. G., Glasmacher, M. A. K., Green, K. D., Ho, Y., Huang, A., Jui, C. C., Kidd, M. J., Kieda, D. B., Knapp, B. C., Ko, S., Larsen, C. G., Lee, W., Loh, E. C., Mannel, E. J., Matthews, J., Matthews, J. N., Newport, B. J., Nitz, D. F., Ong, R. A., Simpson, K. M., Smith, J. D., Sinclair, D., Sokalsky, P., Sommers, P., Song, C., Tang, J. K. K,, Thomas, S. B., van der Velde, J. C., Wiencke, L. R., Wilkinson, C. R., Yoshida, S. & Zhang, X. Z. (2000). Evidence for changing of cosmic ray composition between 10(17) and 10(18) eV from multicomponent measurements. Physical Review Letters, 84(19), 4276-9.
Rights Management (c) American Physical Society
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Identifier ir-main,5042
ARK ark:/87278/s68k7tf8
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ID 704714
Reference URL https://collections.lib.utah.edu/ark:/87278/s68k7tf8
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