Real-time cosmic ray monitoring system for space weather

被引：46

作者：

Kuwabara, T. ^{[1
]}

Bieber, J. W.

Clem, J.

Evenson, P.

Pyle, R.

Munakata, K.

Yasue, S.

Kato, C.

Akahane, S.

Koyama, M.

Fujii, Z.

Duldig, M. L.

Humble, J. E.

Silva, M. R.

Trivedi, N. B.

Gonzalez, W. D.

Schuch, N. J.

机构：

[1] Univ Delaware, Bartol Res Inst, Newark, DE 19716 USA

[2] Univ Delaware, Dept Phys & Astron, Newark, DE 19716 USA

[3] Shinshu Univ, Dept Phys, Matsumoto, Nagano 3908621, Japan

[4] Nagoya Univ, Solar Terr Environm Lab, Nagoya, Aichi 4648601, Japan

[5] Australian Antarctic Div, Kingston, Tas 7050, Australia

[6] Univ Tasmania, Sch Math & Phys, Hobart, Tas 7001, Australia

[7] Natl Inst Space Res, So Reg Space Res Ctr, BR-97105900 Santa Maria, RS, Brazil

来源：

SPACE WEATHER-THE INTERNATIONAL JOURNAL OF RESEARCH AND APPLICATIONS | 2006年 / 4卷 / 08期

关键词：

D O I：

10.1029/2005SW000204

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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.

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