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Institution

California State University, Dominguez Hills

EducationCarson, California, United States
About: California State University, Dominguez Hills is a education organization based out in Carson, California, United States. It is known for research contribution in the topics: Population & Liquidity preference. The organization has 855 authors who have published 1827 publications receiving 46542 citations. The organization is also known as: CSUDH & Dominguez Hills State University.


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Journal ArticleDOI
TL;DR: In this paper, the authors evaluated the severity of meteorological, agricultural, and hydrological forms of drought using six weighted evaluation criteria: robustness, tractability, transparency, sophistication, extendability, and dimensionality.
Abstract: Indices for objectively quantifying the severity of meteorological, agricultural, and hydrological forms of drought are discussed. Indices for each drought form are judged according to six weighted evaluation criteria: robustness, tractability, transparency, sophistication, extendability, and dimensionality. The indices considered most promising for succinctly summarizing drought severity are computed for two climate divisions in Oregon for 24 water years, 1976-99. The assessment determined that the most valuable indices for characterizing meteorological, hydrological, and agricultural droughts are rainfall deciles, total water deficit, and computed soil moisture, respectively.

1,019 citations

Journal ArticleDOI
Y. Fukuda1, M. Ishitsuka1, Yoshitaka Itow1, Takaaki Kajita1, J. Kameda1, K. Kaneyuki1, K. Kobayashi1, Yusuke Koshio1, M. Miura1, S. Moriyama1, Masayuki Nakahata1, S. Nakayama1, A. Okada1, N. Sakurai1, Masato Shiozawa1, Yoshihiro Suzuki1, H. Takeuchi1, Y. Takeuchi1, T. Toshito1, Y. Totsuka1, Shoichi Yamada1, Shantanu Desai2, M. Earl2, E. Kearns2, M. D. Messier2, Kate Scholberg2, Kate Scholberg3, J. L. Stone2, L. R. Sulak2, C. W. Walter2, M. Goldhaber4, T. Barszczak5, David William Casper5, W. Gajewski5, W. R. Kropp5, S. Mine5, D. W. Liu5, L. R. Price5, M. B. Smy5, Henry W. Sobel5, M. R. Vagins5, Todd Haines5, D. Kielczewska5, K. S. Ganezer6, W. E. Keig6, R. W. Ellsworth7, S. Tasaka8, A. Kibayashi, John G. Learned, S. Matsuno, D. Takemori, Y. Hayato, T. Ishii, Takashi Kobayashi, Koji Nakamura, Y. Obayashi, Y. Oyama, A. Sakai, Makoto Sakuda, M. Kohama9, Atsumu Suzuki9, T. Inagaki10, Tsuyoshi Nakaya10, K. Nishikawa10, E. Blaufuss11, S. Dazeley11, R. Svoboda11, J. A. Goodman12, G. Guillian12, G. W. Sullivan12, D. Turcan12, Alec Habig13, J. Hill14, C. K. Jung14, K. Martens15, K. Martens14, Magdalena Malek14, C. Mauger14, C. McGrew14, E. Sharkey14, B. Viren14, C. Yanagisawa14, C. Mitsuda16, K. Miyano16, C. Saji16, T. Shibata16, Y. Kajiyama17, Y. Nagashima17, K. Nitta17, M. Takita17, Minoru Yoshida17, Heekyong Kim18, Soo-Bong Kim18, J. Yoo18, H. Okazawa, T. Ishizuka19, M. Etoh20, Y. Gando20, Takehisa Hasegawa20, Kunio Inoue20, K. Ishihara20, Tomoyuki Maruyama20, J. Shirai20, A. Suzuki20, Masatoshi Koshiba1, Y. Hatakeyama21, Y. Ichikawa21, M. Koike21, Kyoshi Nishijima21, H. Fujiyasu22, Hirokazu Ishino22, M. Morii22, Y. Watanabe22, U. Golebiewska23, S. C. Boyd24, A. L. Stachyra24, R. J. Wilkes24, B. Lee 
TL;DR: Solar neutrino measurements from 1258 days of data from the Super-Kamiokande detector are presented and the recoil electron energy spectrum is consistent with no spectral distortion.
Abstract: Solar neutrino measurements from 1258days of data from the Super-Kamiokande detector are presented. The measurements are based on recoil electrons in the energy range 5.0{endash}20.0MeV. The measured solar neutrino flux is 2.32{+-}0.03(stat){sup +0.08}{sub {minus}0.07}(syst){times}10{sup 6} cm{sup {minus}2}s{sup {minus}1} , which is 45.1{+-}0.5(stat ){sup +1.6}{sub {minus}1.4}(syst) % of that predicted by the BP2000 SSM. The day vs night flux asymmetry ({Phi}{sub n}{minus}{Phi}{sub d})/ {Phi}{sub average} is 0.033{+-}0.022(stat){sup +0.013}{sub {minus}0.012}(syst) . The recoil electron energy spectrum is consistent with no spectral distortion. For the hep neutrino flux, we set a 90% C.L.upper limit of 40{times}10{sup 3} cm{sup {minus}2}s{sup {minus}1} , which is 4.3times the BP2000 SSM prediction.

878 citations

Journal ArticleDOI
S. Fukuda1, Y. Fukuda1, T. Hayakawa1, E. Ichihara1  +183 moreInstitutions (28)
TL;DR: Super-Kamiokande is the world's largest water Cherenkov detector, with net mass 50,000 tons as discussed by the authors, which collected 1678 live-days of data, observing neutrinos from the Sun, Earth's atmosphere, and the K2K long-baseline neutrino beam with high efficiency.
Abstract: Super-Kamiokande is the world's largest water Cherenkov detector, with net mass 50,000 tons. During the period April, 1996 to July, 2001, Super-Kamiokande I collected 1678 live-days of data, observing neutrinos from the Sun, Earth's atmosphere, and the K2K long-baseline neutrino beam with high efficiency. These data provided crucial information for our current understanding of neutrino oscillations, as well as setting stringent limits on nucleon decay. In this paper, we describe the detector in detail, including its site, configuration, data acquisition equipment, online and offline software, and calibration systems which were used during Super-Kamiokande I.

708 citations

Journal ArticleDOI
Y. Ashie1, J. Hosaka1, K. Ishihara1, Yoshitaka Itow1, J. Kameda1, Yusuke Koshio1, A. Minamino1, C. Mitsuda1, M. Miura1, Shigetaka Moriyama1, Masayuki Nakahata1, Toshio Namba1, R. Nambu1, Y. Obayashi1, Masato Shiozawa1, Yoshihiro Suzuki1, Y. Takeuchi1, K. Taki1, Shinya Yamada1, M. Ishitsuka1, Takaaki Kajita1, K. Kaneyuki1, Shoei Nakayama1, A. Okada1, Ko Okumura1, C. Saji1, Y. Takenaga1, S. Clark2, Shantanu Desai2, E. Kearns2, S. Likhoded2, J. L. Stone2, L. R. Sulak2, W. Wang2, M. Goldhaber3, David William Casper4, J. P. Cravens4, W. Gajewski4, W. R. Kropp4, D. W. Liu4, S. Mine4, Michael B. Smy4, Henry W. Sobel4, C. W. Sterner4, Mark R. Vagins4, K. S. Ganezer5, John Hill5, W. E. Keig5, J. S. Jang6, J. Y. Kim6, I. T. Lim6, Kate Scholberg7, C. W. Walter7, R. W. Ellsworth8, S. Tasaka9, G. Guillian, A. Kibayashi, John G. Learned, S. Matsuno, D. Takemori, M. D. Messier10, Y. Hayato, A. K. Ichikawa, T. Ishida, T. Ishii, T. Iwashita, Takashi Kobayashi, T. Maruyama11, Koji Nakamura, K. Nitta, Yuichi Oyama, Makoto Sakuda12, Y. Totsuka, Atsumu Suzuki13, Masaya Hasegawa14, K. Hayashi14, I. Kato14, H. Maesaka14, Taichi Morita14, Tsuyoshi Nakaya14, K. Nishikawa14, T. Sasaki14, S. Ueda14, Shoji Yamamoto14, Todd Haines4, Todd Haines15, S. Dazeley16, S. Hatakeyama16, R. Svoboda16, E. Blaufuss17, J. A. Goodman17, G. W. Sullivan17, D. Turcan17, Alec Habig18, Y. Fukuda19, C. K. Jung20, T. Kato20, Katsuhiro Kobayashi20, Magdalena Malek20, C. Mauger20, C. McGrew20, A. Sarrat20, E. Sharkey20, C. Yanagisawa20, T. Toshito21, Kazumasa Miyano22, N. Tamura22, J. Ishii23, Y. Kuno23, Minoru Yoshida23, S. B. Kim24, J. Yoo24, H. Okazawa, T. Ishizuka25, Y. Choi26, H. Seo26, Y. Gando27, Takehisa Hasegawa27, Kunio Inoue27, J. Shirai27, A. Suzuki27, Masatoshi Koshiba1, Y. Nakajima28, Kyoshi Nishijima28, T. Harada29, Hirokazu Ishino29, Y. Watanabe29, D. Kielczewska30, D. Kielczewska4, J. Zalipska30, H. G. Berns31, R. Gran31, K. K. Shiraishi31, A. L. Stachyra31, K. Washburn31, R. J. Wilkes31 
TL;DR: In this article, a combined analysis of fully-contained, partially-contained and upward-going muon atmospheric neutrino data from a 1489 d exposure of the Super-Kamiokande detector is presented.
Abstract: We present a combined analysis of fully-contained, partially-contained and upward-going muon atmospheric neutrino data from a 1489 d exposure of the Super-Kamiokande detector. The data samples span roughly five decades in neutrino energy, from 100 MeV to 10 TeV. A detailed Monte Carlo comparison is described and presented. The data is fit to the Monte Carlo expectation, and is found to be consistent with neutrino oscillations of {nu}{sub {mu}}{r_reversible}{nu}{sub {tau}} with sin{sup 2}2{theta}>0.92 and 1.5x10{sup -3}<{delta}m{sup 2}<3.4x10{sup -3} eV{sup 2} at 90% confidence level.

701 citations

Journal ArticleDOI
S. Fukuda1, Y. Fukuda1, M. Ishitsuka1, Yoshitaka Itow1, Takaaki Kajita1, J. Kameda1, K. Kaneyuki1, K. Kobayashi1, Yusuke Koshio1, M. Miura1, S. Moriyama1, Masayuki Nakahata1, S. Nakayama1, Toshio Namba1, A. Okada1, N. Sakurai1, Masato Shiozawa1, Yoshihiro Suzuki1, H. Takeuchi1, Y. Takeuchi1, Y. Totsuka1, Shoichi Yamada1, Shantanu Desai2, M. Earl2, E. Kearns2, M. D. Messier2, J. L. Stone2, L. R. Sulak2, C. W. Walter2, M. Goldhaber3, T. Barszczak4, David William Casper4, W. Gajewski4, W. R. Kropp4, S. Mine4, D. W. Liu4, M. B. Smy4, Henry W. Sobel4, M. R. Vagins4, A. M. Gago5, K. S. Ganezer5, W. E. Keig5, R. W. Ellsworth6, S. Tasaka7, A. Kibayashi8, John G. Learned8, S. Matsuno8, D. Takemori8, Y. Hayato9, T. Ishii9, Takashi Kobayashi9, T. Maruyama9, Koji Nakamura9, Y. Obayashi1, Y. Obayashi9, Y. Oyama9, Makoto Sakuda9, Minoru Yoshida9, M. Kohama10, T. Iwashita10, Atsumu Suzuki10, A. K. Ichikawa9, A. K. Ichikawa11, T. Inagaki11, I. Kato11, Tsuyoshi Nakaya11, K. Nishikawa11, Todd Haines4, Todd Haines12, S. Dazeley13, S. Hatakeyama13, R. Svoboda13, E. Blaufuss14, M. L. Chen14, J. A. Goodman14, G. Guillian14, G. W. Sullivan14, D. Turč14, Kate Scholberg15, Alec Habig16, M. Ackermann17, J. Hill17, C. K. Jung17, Magdalena Malek17, K. Martens17, C. Mauger17, C. McGrew17, E. Sharkey17, B. Viren3, B. Viren17, C. Yanagisawa17, T. Toshito18, C. Mitsuda19, K. Miyano19, C. Saji19, T. Shibata19, Y. Kajiyama20, Y. Nagashima20, K. Nitta20, M. Takita20, Hyosun Kim21, S. B. Kim21, J. Yoo21, H. Okazawa, T. Ishizuka22, M. Etoh23, Y. Gando23, Takehisa Hasegawa23, Kunio Inoue23, K. Ishihara23, J. Shirai23, A. Suzuki23, Masatoshi Koshiba1, Y. Hatakeyama24, Y. Ichikawa24, M. Koike24, Kyoshi Nishijima24, Hirokazu Ishino25, Mikio Morii25, R. Nishimura25, Y. Watanabe25, D. Kielczewska4, D. Kielczewska26, H. G. Berns27, S. C. Boyd27, A. L. Stachyra27, R. J. Wilkes27 
TL;DR: In this paper, a number of different fits to solar neutrino mixing and mass square difference were performed using 1496 days of Super-Kamiokande-I's solar NE data.

680 citations


Authors

Showing all 881 results

NameH-indexPapersCitations
B. P. Crill148486111895
Danny Miller13351271238
John Hill13181579034
Philip P. Power9066533211
A. M. Gago8834723799
Masashi Yokoyama7331018817
K. S. Ganezer6814016304
James C. Fettinger6249215698
Carl K. Hoh6119211149
Gary J. Long5437512432
Miguel A. Garcia-Garibay502638287
J. W. Price492038503
M. Osipenko483048585
Luis M. Campos451429721
W. E. Keig445910215
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Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
20237
202229
2021157
2020151
2019118
2018126