Zobrazeno 1 - 10
of 33
pro vyhledávání: '"C. Jake Waddington"'
Autor:
A. W. Labrador, G. E. Simburger, Makoto Sasaki, S. L. Nutter, G. A. deNolfo, Grant Mitchell, J. H. Buckley, Zachary Hughes, K. Sakai, T. J. Brandt, John Krizmanic, Teresa Tatoli, I. Liceaga-Indart, Jeff Dumonthier, Dana Braun, M. H. Israel, Jason Link, C. Jake Waddington, Y. Akaike, Mark E. Wiedenbeck, Richard Bose, Martin Olevitch, John Mitchell, W. Robert Binns, George Suarez, Brian Rauch, R. A. Mewaldt, E. C. Stone, Nathan Elliot Walsh, Paul Dowkontt
Publikováno v:
Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019).
The response to 150 GeV/nuc primary lead ($^{208}$Pb) and fragmented (A/Z=2.4, 2.2, 2.0) beams measured a silicon strip detector, designed for use in the Heavy Nuclei eXplorer (HNX) and an upgrade of the Super Trans-Iron Galactic Element Recorder (Su
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a8f501f3e5ff688b974cd2247559cc71
https://doi.org/10.22323/1.358.0094
https://doi.org/10.22323/1.358.0094
Autor:
C. Jake Waddington
Publikováno v:
New Astronomy Reviews. 42:277-286
A survey of the present state of attempts to deduce the abundances of nuclei at the sources of the cosmic radiation from the abundances measured near the earth. Particular attention is directed towards the effects that are introduced by the energy-de
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5dc1685b3fe8ff8b1c9766ae5e6f2234
https://doi.org/10.1016/s1387-6473(98)00013-x
https://doi.org/10.1016/s1387-6473(98)00013-x
Autor:
C. Jake Waddington
Publikováno v:
Advances in Space Research. 19:759-762
A weighted slab approximation to a leaky box model has been developed to study the influence of various parameters and cross sections on the propagation of Z > 28 ultraheavy (UH) cosmic ray nuclei from the source to earth. This model starts with nucl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0562c504e1f951d3e5664994a258e60b
https://doi.org/10.1016/s0273-1177(96)00142-1
https://doi.org/10.1016/s0273-1177(96)00142-1
Autor:
C. Jake Waddington
Publikováno v:
International Journal of Modern Physics E. :739-766
Preliminary results are described from three separate experiments observing the interactions of gold nuclei accelerated to 10.6 GeV/nucleon at the Brookhaven AGS. Nuclear emulsion results present a global picture of the various interaction modes and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::da24dbaaaad9fc4b8664b240315825fc
https://doi.org/10.1142/s0218301393000327
https://doi.org/10.1142/s0218301393000327
Autor:
C. Jake Waddington
Publikováno v:
AIP Conference Proceedings.
A study has been made of the sensitivity of observations of the elemental abundances of those nuclei just heavier than 28Ni to assumptions concerning propagation and source abundances. Calculations of the propagation of elements with 42⩾Z⩾27 have
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e3e676df48cfb0fddf468e599af0f8e4
https://doi.org/10.1063/1.1324356
https://doi.org/10.1063/1.1324356
Autor:
Robert R. Clinton, C. Jake Waddington
Publikováno v:
AIP Conference Proceedings.
This paper gives a brief description of the current status of our program to develop a modular array of large electronic particle detectors. These modules were designed to study the UH nuclei in the cosmic radiatin with eventual deployment on the Spa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c5c30945088ef104426e1631ef72c387
https://doi.org/10.1063/1.39171
https://doi.org/10.1063/1.39171
Autor:
C. Jake Waddington
Publikováno v:
The Astrophysical Journal. 470:1218
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a434e58c65adbed0667db720123a4b02
https://doi.org/10.1086/177944
https://doi.org/10.1086/177944
Autor:
C. Jake Waddington
Publikováno v:
Physics Today. 46:65-65
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1b12c5dbcb63025521a83e4e059c716f
https://doi.org/10.1063/1.2809137
https://doi.org/10.1063/1.2809137
Publikováno v:
Physical Review D. 25:2341-2350
We use low-energy data on pion production in collisions between nuclei to study some characteristics of high-energy cosmic-ray showers. The fact that pion production is suppressed in collisions initiated by heavy nuclei has the result that fluctuatio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::af826f4ca6e55c0677939c0b587a73bf
https://doi.org/10.1103/physrevd.25.2341
https://doi.org/10.1103/physrevd.25.2341
Publikováno v:
Physics Today. 28:23-31
Ultraheavy cosmic‐ray nuclei, those with atomic number over thirty, constitute less than about one in 107 of the relativistic particles that stream through our solar system, yet they promise to lead to a major contribution in our understanding of t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2ab005ecc8e43e5286eee61627cc3c75
https://doi.org/10.1063/1.3068964
https://doi.org/10.1063/1.3068964