Solar neutron event associated with an X8.3 flare on 2003 November 2

K. Watanabe; Y. Muraki; Y. Matsubara; T. Sako; A. Velarde; R. Ticona; N. Martinic; P. Miranda; F. Kakimoto; S. Ogio; Y. Tsunesada; H. Tokuno

Solar neutron event associated with an X8.3 flare on 2003 November 2

K. Watanabe, Y. Muraki, Y. Matsubara, T. Sako, A. Velarde, R. Ticona, N. Martinic, P. Miranda, F. Kakimoto, S. Ogio, Y. Tsunesada, H. Tokuno

Research output: Contribution to conference › Paper › peer-review

1 Scopus citations

Abstract

On November 2, 2003, in association with X8.3 flare, a solar neutron event was detected with high statistical significance (4.7 σ) by the neutron monitor at Mt. Chacaltaya, Bolivia. Although large GLE event occurred and was observed by many neutron monitors in association with this flare, the start time of the neutron event was earlier than that of the GLE event. At this flare, the intense emission of γ-rays has been observed by the RHESSI satellite. The production time of solar neutrons was well correlated with those of γ-rays.

Original language	English
Pages	29-32
Number of pages	4
State	Published - 2005
Event	29th International Cosmic Ray Conference, ICRC 2005 - Pune, India Duration: 3 Aug 2005 → 10 Aug 2005

Conference

Conference	29th International Cosmic Ray Conference, ICRC 2005
Country/Territory	India
City	Pune
Period	3/08/05 → 10/08/05

Cite this

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title = "Solar neutron event associated with an X8.3 flare on 2003 November 2",

abstract = "On November 2, 2003, in association with X8.3 flare, a solar neutron event was detected with high statistical significance (4.7 σ) by the neutron monitor at Mt. Chacaltaya, Bolivia. Although large GLE event occurred and was observed by many neutron monitors in association with this flare, the start time of the neutron event was earlier than that of the GLE event. At this flare, the intense emission of γ-rays has been observed by the RHESSI satellite. The production time of solar neutrons was well correlated with those of γ-rays.",

author = "K. Watanabe and Y. Muraki and Y. Matsubara and T. Sako and A. Velarde and R. Ticona and N. Martinic and P. Miranda and F. Kakimoto and S. Ogio and Y. Tsunesada and H. Tokuno",

year = "2005",

language = "Ingl{\'e}s",

pages = "29--32",

note = "29th International Cosmic Ray Conference, ICRC 2005 ; Conference date: 03-08-2005 Through 10-08-2005",

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TY - CONF

T1 - Solar neutron event associated with an X8.3 flare on 2003 November 2

AU - Watanabe, K.

AU - Muraki, Y.

AU - Matsubara, Y.

AU - Sako, T.

AU - Velarde, A.

AU - Ticona, R.

AU - Martinic, N.

AU - Miranda, P.

AU - Kakimoto, F.

AU - Ogio, S.

AU - Tsunesada, Y.

AU - Tokuno, H.

PY - 2005

Y1 - 2005

N2 - On November 2, 2003, in association with X8.3 flare, a solar neutron event was detected with high statistical significance (4.7 σ) by the neutron monitor at Mt. Chacaltaya, Bolivia. Although large GLE event occurred and was observed by many neutron monitors in association with this flare, the start time of the neutron event was earlier than that of the GLE event. At this flare, the intense emission of γ-rays has been observed by the RHESSI satellite. The production time of solar neutrons was well correlated with those of γ-rays.

AB - On November 2, 2003, in association with X8.3 flare, a solar neutron event was detected with high statistical significance (4.7 σ) by the neutron monitor at Mt. Chacaltaya, Bolivia. Although large GLE event occurred and was observed by many neutron monitors in association with this flare, the start time of the neutron event was earlier than that of the GLE event. At this flare, the intense emission of γ-rays has been observed by the RHESSI satellite. The production time of solar neutrons was well correlated with those of γ-rays.

UR - http://www.scopus.com/inward/record.url?scp=84899026428&partnerID=8YFLogxK

M3 - Artículo

AN - SCOPUS:84899026428

SP - 29

EP - 32

T2 - 29th International Cosmic Ray Conference, ICRC 2005

Y2 - 3 August 2005 through 10 August 2005

ER -

Solar neutron event associated with an X8.3 flare on 2003 November 2

Abstract

Conference

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