Hostname: page-component-77c89778f8-vsgnj Total loading time: 0 Render date: 2024-07-18T18:23:58.109Z Has data issue: false hasContentIssue false

Solar Neutron Observations During the Coming Solar Maximum: A Plan on the Japan-China Collaborative Project

Published online by Cambridge University Press:  27 September 2017

Kunitomo Sakurai*
Affiliation:
Institute of Physics, kanagawa University Rokkakubashi, Yokohama 221, Japan

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Neutrons are sometimes released from solar flares accompanied by generation of high energy protons and other nuclei and some of them occasionally reach the earth before they decay radioactively. Together with the satellite observations on gamma ray and neutron emissions associated with such flares, the ground-based observations of these neutrons give us a clue to understand the possible nuclear interactions of those protons and nuclei with gases ambient in the solar atmosphere. A review is given on the Japan-China collaborative program on the ground-based observations of these neutrons for the coming solar maximum, though there still remain obstacles to be resolved.

Type
Session II: Solar Flares
Copyright
Copyright © Kluwer 1989

References

Chupp, E., Ann. Rev. Astron. Astrophys., 22, 359 (1984).Google Scholar
Chupp, E., Forrest, D.J., Higbie, P.R., Suri, A. and Tsai, C., Nature, 241, 333 (1972).Google Scholar
Debrunner, H., Fluckiger, , Chupp, E.L. and Forrest, D.J., Proc. 18th Intcrnatl. Cosmic Ray Conf., Bangalore, SP 3, 257 (1983).Google Scholar
Ogawara, Y., Solar. Phys., 113, 361 (1987).Google Scholar
Ramaty, R., Kozlovsky, B. and Lingenfelter, R.E., Astrophys. J. Suppl. 40, 487 (1979).Google Scholar
Sakurai, K., Physics of Solar Cosmic Rays, Univ. of Tokyo Press, Tokyo (1974).Google Scholar
Takahashi, K., Space Sci. Reviews (in press, 1988).Google Scholar