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Global Muon Detector Network Used for Space Weather Applications
Authors:M Rockenbach  A Dal Lago  N J Schuch  K Munakata  T Kuwabara  A G Oliveira  E Echer  C R Braga  R R S Mendonça  C Kato  M Kozai  M Tokumaru  J W Bieber  P Evenson  M L Duldig  J E Humble  H K Al Jassar  M M Sharma  I Sabbah
Institution:1. Southern Regional Space Research Center (CRS/INPE), P.O. Box 5021, 97110-970, Santa Maria, RS, Brazil
2. National Institute for Space Research (INPE), 12227, S?o José dos Campos, Brazil
4. Physics Department, Shinshu University, Matsumoto, Nagano, 390-8621, Japan
6. Bartol Research Institute and Department of Physics and Astronomy, University of Delaware, Newark, DE, 19716, USA
3. Instituto de Pesquisa e Desenvolvimento, Universidade do Vale do Paraíba, S?o José dos Campos, Brazil
5. Solar Terrestrial Environment Laboratory, Nagoya University, Nagoya, Aichi, 464-8601, Japan
7. School of Physical Sciences, University of Tasmania, Hobart, Tasmania, 7001, Australia
8. Physics Department, Faculty of Science, Kuwait University, Kuwait city, Kuwait
9. Department of Natural Sciences, College of Health Sciences, Public Authority of Applied Education and Training, Kuwait City, Kuwait
Abstract:In this work, we summarize the development and current status of the Global Muon Detector Network (GMDN). The GMDN started in 1992 with only two muon detectors. It has consisted of four detectors since the Kuwait-city muon hodoscope detector was installed in March 2006. The present network has a total of 60 directional channels with an improved coverage of the sunward Interplanetary Magnetic Field (IMF) orientation, making it possible to continuously monitor cosmic ray precursors of geomagnetic storms. The data analysis methods developed also permit precise calculation of the three dimensional cosmic ray anisotropy on an hourly basis free from the atmospheric temperature effect and analysis of the cosmic ray precursors free from the diurnal anisotropy of the cosmic ray intensity.
Keywords:
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