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Effects of ICMEs on High Energetic Particles as Observed by the Global Muon Detector Network (GMDN)

Published online by Cambridge University Press:  24 July 2018

A. Dal Lago
Affiliation:
National Institute for Space Research (INPE), Avenida dos Astronautas-12227-010, São José dos Campos-SP, Brazil email: alisson.dallago@inpe.br
C. R. Braga
Affiliation:
National Institute for Space Research (INPE), Avenida dos Astronautas-12227-010, São José dos Campos-SP, Brazil email: alisson.dallago@inpe.br
R. R. S. de Mendonca
Affiliation:
National Institute for Space Research (INPE), Avenida dos Astronautas-12227-010, São José dos Campos-SP, Brazil email: alisson.dallago@inpe.br
M. Rockenbach
Affiliation:
National Institute for Space Research (INPE), Avenida dos Astronautas-12227-010, São José dos Campos-SP, Brazil email: alisson.dallago@inpe.br
E. Echer
Affiliation:
National Institute for Space Research (INPE), Avenida dos Astronautas-12227-010, São José dos Campos-SP, Brazil email: alisson.dallago@inpe.br
N. J. Schuch
Affiliation:
Southern Regional Space Research Center - CRS/INPE, Santa Maria, Brazil
K. Munakata
Affiliation:
Shinshu University, Matsumoto, Japan
C. Kato
Affiliation:
Shinshu University, Matsumoto, Japan
T. Kuwabara
Affiliation:
Chiba University, Chiba City, Chiba, Japan
M. Kozai
Affiliation:
Japan Aerospace Exploration Agency - JAXA, Sagamihara, Kanagawa, Japan
H. K. Al Jassar
Affiliation:
Kuwait University, Kuwait City, Kuwait
M. M. Sharma
Affiliation:
Kuwait University, Kuwait City, Kuwait
M. Tokumaru
Affiliation:
Institute for Space-Earth Environmental Research, Nagoya University, Japan
M. Duldig
Affiliation:
University of Tasmania, Hobart, Tasmania, Australia
J. Humble
Affiliation:
University of Tasmania, Hobart, Tasmania, Australia
P. Evenson
Affiliation:
Bartol Research Institute, University of Delaware, Newark, USA
I. Sabbah
Affiliation:
Department of Natural Sciences, College of Health Sciences, Public Authority for Applied Education and Training, Kuwait City, Kuwait
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Abstract

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The Global Muon Detector Network (GMDN) is composed by four ground cosmic ray detectors distributed around the Earth: Nagoya (Japan), Hobart (Australia), Sao Martinho da Serra (Brazil) and Kuwait city (Kuwait). The network has operated since March 2006. It has been upgraded a few times, increasing its detection area. Each detector is sensitive to muons produced by the interactions of ~50 GeV Galactic Cosmic Rays (GCR) with the Earth′s atmosphere. At these energies, GCR are known to be affected by interplanetary disturbances in the vicinity of the earth. Of special interest are the interplanetary counterparts of coronal mass ejections (ICMEs) and their driven shocks because they are known to be the main origins of geomagnetic storms. It has been observed that these ICMEs produce changes in the cosmic ray gradient, which can be measured by GMDN observations. In terms of applications for space weather, some attempts have been made to use GMDN for forecasting ICME arrival at the earth with lead times of the order of few hours. Scientific space weather studies benefit the most from the GMDN network. As an example, studies have been able to determine ICME orientation at the earth using cosmic ray gradient. Such determinations are of crucial importance for southward interplanetary magnetic field estimates, as well as ICME rotation.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2018 

References

Braga, et al. 2011, 32nd International Cosmic Ray Conference, 10, 286, ISBN: 978-1-63439-138-2Google Scholar
Burlaga, L. F., Sittler, E., Mariani, F. & Schwenn, R. 1981, J. Geophys. Res., 86, 6673CrossRefGoogle Scholar
De Mendonca, et al. 2016, ApJ, 830, 88CrossRefGoogle Scholar
Duldig, M. 2000, Space Science Review, 93, 207CrossRefGoogle Scholar
Forbush, S. E. 1937, Physical Review, 51, 12, 1108CrossRefGoogle Scholar
Fushishita, A., et al. 2010, ApJ, 715, 2, 12391247CrossRefGoogle Scholar
Gosling, J. T., McComas, D. J., Phillips, J. L. & Bame, S. J. 1991, J. Geophys. Res., 96, A5, 7831CrossRefGoogle Scholar
Gonzalez, W. D., Echer, E., Tsurutani, B. T., Clua de Gonzalez, A. L. & Dal Lago, A. 2011, SSR, 158, 69Google Scholar
Howard, R. A., et al. 1982, ApJ, 263, 2L, 101CrossRefGoogle Scholar
Kozai, M., Munakata, K., Kato, C., Kuwabara, T., Rockenbach, M., Lago, A. Dal, Schuch, N. J., Braga, C. R., Mendonça, R. R. S., Jassar, H. K. Al, Sharma, M. M., Duldig, M. L., Humble, J. E., Evenson, P., Sabbah, I. & Tokumaru, M. 2016, ApJ, 825, 100CrossRefGoogle Scholar
Kuwabara, T., et al. 2006, Space Weather, 4, 8, S08001Google Scholar
Kuwabara, T., et al. 2009, JGR, 114, A05109CrossRefGoogle Scholar
McDonald, F. B. 2000, Space Science Reviews, 93, 263CrossRefGoogle Scholar
Munakata, K., et al. 2000, JGR, 27457CrossRefGoogle Scholar
Nagashima, K., et al. 1992, Planetary and Space Science, 40, 8, 1109CrossRefGoogle Scholar
Rockenbach, M., et al. 2011, GRL, 38, L16108CrossRefGoogle Scholar
Schwenn, R. 1996, Astrophys. Space Sci., 243, 1, 187CrossRefGoogle Scholar
Schwenn, R., Dal Lago, A., Huttunen, E. & Gonzalez, W. D. 2005, Ann. Geophys., 23, AG/2004180, 1033CrossRefGoogle Scholar
Simpson, J. A. 1954, Physical Review, 94, 2, 426CrossRefGoogle Scholar
Szajko, N. S., Cristiani, G., Mandrini, C. H. & Dal Lago, A. 2013, ASR, 51, 10, 1842Google Scholar