%0 Journal Article
%@holdercode {isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S}
%@nexthigherunit 8JMKD3MGPCW/3EU29DP 8JMKD3MGPCW/3EUFCFP
%@archivingpolicy denypublisher denyfinaldraft
%N 8
%@secondarytype PRE PI
%@usergroup administrator
%@usergroup simone
%P S08001
%4 sid.inpe.br/mtc-m16@80/2006/11.22.13.56
%X We have developed a real-time system to monitor high-energy cosmic rays for use in space weather forecasting and specification. Neutron monitors and muon detectors are used for our system, making it possible to observe cosmic rays with dual energy range observations. In large solar energetic particle (SEP) events, the ground level enhancement (GLE) can provide the earliest alert for the onset of the SEP event. The loss cone precursor anisotropy predicts the arrival of interplanetary shocks and the associated interplanetary coronal mass ejections (ICMEs), while the occurrence of bidirectional cosmic ray streaming indicates that Earth is within a large ICME. This article describes a set of real-time Web displays that clearly show the appearance of the GLE, loss cone precursor, and other space weather phenomena related to cosmic rays.
%8 Aug.
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%@group RSU-INPE-MCT-BR
%@group RSU-INPE-MCT-BR
%@group DGE-INPE-MCT-BR
%@group RSU-INPE-MCT-BR
%@issn 1539-4956
%@affiliation Bartol Research Institute and Departament of Physics and Astronomy, University of Delaware, Newark, Delaware, USA
%@affiliation Bartol Research Institute and Departament of Physics and Astronomy, University of Delaware, Newark, Delaware, USA
%@affiliation Bartol Research Institute and Departament of Physics and Astronomy, University of Delaware, Newark, Delaware, USA
%@affiliation Bartol Research Institute and Departament of Physics and Astronomy, University of Delaware, Newark, Delaware, USA
%@affiliation Bartol Research Institute and Departament of Physics and Astronomy, University of Delaware, Newark, Delaware, USA
%@affiliation Physics Department, Shinshu University, Matsumoto, Japan
%@affiliation Physics Department, Shinshu University, Matsumoto, Japan
%@affiliation Physics Department, Shinshu University, Matsumoto, Japan
%@affiliation Physics Department, Shinshu University, Matsumoto, Japan
%@affiliation Physics Department, Shinshu University, Matsumoto, Japan
%@affiliation Solar Terrestrial Environment  Laboratory, Nagoya University, Nagoya Japan
%@affiliation Australian Antarctic Division, Kingston, Tasmania, Australia
%@affiliation School of Mathematics and Physics, University of Tasmania, Australia
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%D 2006
%A Kuwabara, T.,
%A Bieber, J. W.,
%A Clem, J.,
%A Evenson, P.,
%A Pyle, R.,
%A Munakata, K.,
%A Yasue, S.,
%A Kato, C.,
%A Akahane, S.,
%A Koyama, M.,
%A Fujii, Z.,
%A Duldig, M. L.,
%A Humble, J. E.,
%A Silva, Marlos Rockenbach da,
%A Trivedi, Nalin Babulal,
%A Alarcon, Walter Demétrio Gonzalez,
%A Schuch,  Nelson Jorge,
%@area CEA
%T Real-time cosmic ray monitoring system for space weather
%@electronicmailaddress takao@bartol.udel.edu
%B Space Weather
%@versiontype publisher
%V 4
%@dissemination WEBSCI
%K CORONAL MASS EJECTIONS, MUON DETECTOR NETWORK, GEOMAGNETIC STORMS, FORBUSH DECREASES, CME-GEOMETRY, ANISOTROPY, PRECURSORS, SHOCK.
%@secondarykey INPE--PRE/
%2 sid.inpe.br/mtc-m16@80/2006/11.22.13.56.48
%@documentstage not transferred
%@doi 10.1029/2005SW000204