Solar flare and neutron telescope

Y. Muraki, Y. Matsubara, I. Imaida, T. Koi, T. Murata, A. Okada, S. Sakakibara, T. Sako, H. Tsuchiya, Y. Munakata, S. Shibata, R. Tatsuoka, H. Sakai, T. Nonaka, T. Ohnishi, T. Wakasa, K. Hatanaka, Y. Ishida

Research output: Contribution to journalArticle

1 Citation (Scopus)

Abstract

For the solar neutron event of June 3rd,1982, a new interpretation is given on ion acceleration mechanisms at the solar surface. The event can be explained by the impulsive acceleration of ions just after electron acceleration. For the June 4th,1991 solar neutron event, discrepancies in the absolute solar neutron fluxes measured by three different detectors are investigated using neutron beams at RCNP, Osaka university. We propose here an interpretation which explains all data consistently based on the premise that solar neutrons generate many low energy neutrons in the atmosphere by internuclear cascade processes.

Original languageEnglish
Pages (from-to)3-11
Number of pages9
JournalNuclear Physics B - Proceedings Supplements
Volume60
Issue number3
DOIs
Publication statusPublished - Jan 1998

Fingerprint

solar neutrons
solar flares
telescopes
electron acceleration
neutron beams
flux (rate)
cascades
ions
neutrons
atmospheres
detectors

All Science Journal Classification (ASJC) codes

  • Atomic and Molecular Physics, and Optics
  • Nuclear and High Energy Physics

Cite this

Muraki, Y., Matsubara, Y., Imaida, I., Koi, T., Murata, T., Okada, A., ... Ishida, Y. (1998). Solar flare and neutron telescope. Nuclear Physics B - Proceedings Supplements, 60(3), 3-11. https://doi.org/10.1016/S0920-5632(97)00496-9

Solar flare and neutron telescope. / Muraki, Y.; Matsubara, Y.; Imaida, I.; Koi, T.; Murata, T.; Okada, A.; Sakakibara, S.; Sako, T.; Tsuchiya, H.; Munakata, Y.; Shibata, S.; Tatsuoka, R.; Sakai, H.; Nonaka, T.; Ohnishi, T.; Wakasa, T.; Hatanaka, K.; Ishida, Y.

In: Nuclear Physics B - Proceedings Supplements, Vol. 60, No. 3, 01.1998, p. 3-11.

Research output: Contribution to journalArticle

Muraki, Y, Matsubara, Y, Imaida, I, Koi, T, Murata, T, Okada, A, Sakakibara, S, Sako, T, Tsuchiya, H, Munakata, Y, Shibata, S, Tatsuoka, R, Sakai, H, Nonaka, T, Ohnishi, T, Wakasa, T, Hatanaka, K & Ishida, Y 1998, 'Solar flare and neutron telescope', Nuclear Physics B - Proceedings Supplements, vol. 60, no. 3, pp. 3-11. https://doi.org/10.1016/S0920-5632(97)00496-9
Muraki Y, Matsubara Y, Imaida I, Koi T, Murata T, Okada A et al. Solar flare and neutron telescope. Nuclear Physics B - Proceedings Supplements. 1998 Jan;60(3):3-11. https://doi.org/10.1016/S0920-5632(97)00496-9
Muraki, Y. ; Matsubara, Y. ; Imaida, I. ; Koi, T. ; Murata, T. ; Okada, A. ; Sakakibara, S. ; Sako, T. ; Tsuchiya, H. ; Munakata, Y. ; Shibata, S. ; Tatsuoka, R. ; Sakai, H. ; Nonaka, T. ; Ohnishi, T. ; Wakasa, T. ; Hatanaka, K. ; Ishida, Y. / Solar flare and neutron telescope. In: Nuclear Physics B - Proceedings Supplements. 1998 ; Vol. 60, No. 3. pp. 3-11.
@article{c2783aacb27a4efaa759069ca924fa49,
title = "Solar flare and neutron telescope",
abstract = "For the solar neutron event of June 3rd,1982, a new interpretation is given on ion acceleration mechanisms at the solar surface. The event can be explained by the impulsive acceleration of ions just after electron acceleration. For the June 4th,1991 solar neutron event, discrepancies in the absolute solar neutron fluxes measured by three different detectors are investigated using neutron beams at RCNP, Osaka university. We propose here an interpretation which explains all data consistently based on the premise that solar neutrons generate many low energy neutrons in the atmosphere by internuclear cascade processes.",
author = "Y. Muraki and Y. Matsubara and I. Imaida and T. Koi and T. Murata and A. Okada and S. Sakakibara and T. Sako and H. Tsuchiya and Y. Munakata and S. Shibata and R. Tatsuoka and H. Sakai and T. Nonaka and T. Ohnishi and T. Wakasa and K. Hatanaka and Y. Ishida",
year = "1998",
month = "1",
doi = "10.1016/S0920-5632(97)00496-9",
language = "English",
volume = "60",
pages = "3--11",
journal = "Nuclear and Particle Physics Proceedings",
issn = "2405-6014",
publisher = "Elsevier",
number = "3",

}

TY - JOUR

T1 - Solar flare and neutron telescope

AU - Muraki, Y.

AU - Matsubara, Y.

AU - Imaida, I.

AU - Koi, T.

AU - Murata, T.

AU - Okada, A.

AU - Sakakibara, S.

AU - Sako, T.

AU - Tsuchiya, H.

AU - Munakata, Y.

AU - Shibata, S.

AU - Tatsuoka, R.

AU - Sakai, H.

AU - Nonaka, T.

AU - Ohnishi, T.

AU - Wakasa, T.

AU - Hatanaka, K.

AU - Ishida, Y.

PY - 1998/1

Y1 - 1998/1

N2 - For the solar neutron event of June 3rd,1982, a new interpretation is given on ion acceleration mechanisms at the solar surface. The event can be explained by the impulsive acceleration of ions just after electron acceleration. For the June 4th,1991 solar neutron event, discrepancies in the absolute solar neutron fluxes measured by three different detectors are investigated using neutron beams at RCNP, Osaka university. We propose here an interpretation which explains all data consistently based on the premise that solar neutrons generate many low energy neutrons in the atmosphere by internuclear cascade processes.

AB - For the solar neutron event of June 3rd,1982, a new interpretation is given on ion acceleration mechanisms at the solar surface. The event can be explained by the impulsive acceleration of ions just after electron acceleration. For the June 4th,1991 solar neutron event, discrepancies in the absolute solar neutron fluxes measured by three different detectors are investigated using neutron beams at RCNP, Osaka university. We propose here an interpretation which explains all data consistently based on the premise that solar neutrons generate many low energy neutrons in the atmosphere by internuclear cascade processes.

UR - http://www.scopus.com/inward/record.url?scp=0031603078&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=0031603078&partnerID=8YFLogxK

U2 - 10.1016/S0920-5632(97)00496-9

DO - 10.1016/S0920-5632(97)00496-9

M3 - Article

AN - SCOPUS:0031603078

VL - 60

SP - 3

EP - 11

JO - Nuclear and Particle Physics Proceedings

JF - Nuclear and Particle Physics Proceedings

SN - 2405-6014

IS - 3

ER -