Status of the world-wide network of solar neutron telescopes in solar cycle 24

Y. Matsubara; Y. Muraki; T. Sako; Y. Itow; T. Sakai; S. Shibata; T. Yuda; M. Ohnishi; H. Tsuchiya; Y. Katayose; K. Namikawa; R. Ogasawara; Y. Mizumoto; F. Kakimoto; Y. Tsunesada; K. Watanabe; E. Flückiger; R. Bütikofer; A. Chilingarian; G. Hovsepyan; Y. Tan; J. L. Zhang; R. Ticona; W. Tavera; P. Miranda; J. Valdes-Galicia; L. X. Gonzalez; A. Hurtado; O. Musalem

Status of the world-wide network of solar neutron telescopes in solar cycle 24

Y. Matsubara, Y. Muraki, T. Sako, Y. Itow, T. Sakai, S. Shibata, T. Yuda, M. Ohnishi, H. Tsuchiya, Y. Katayose, K. Namikawa, R. Ogasawara, Y. Mizumoto, F. Kakimoto, Y. Tsunesada, K. Watanabe, E. Flückiger, R. Bütikofer, A. Chilingarian, G. HovsepyanY. Tan, J. L. Zhang, R. Ticona, W. Tavera, P. Miranda, J. Valdes-Galicia, L. X. Gonzalez, A. Hurtado, O. Musalem

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

1 Scopus citations

Abstract

A network of solar neutron telescopes has been developed since the middle of solar cycle 22. We have detected several important solar neutron events until the end of solar cycle 23 using solar neutron telescopes, but the accumulation of more solar neutron events is indispensable to eclucidate the acceleration mechanism of high energy particles. The data of the solar magnetic field with a space resolution of 0.3 arcsec obtained by Hinode satellite will be useful to understand solar neutron events more efficiently than during the previous solar cycles. In this paper we discuss the expected scientific results obtained by the world-wide network of solar neutron telescopes during solar cycle 24.

Original language	English
State	Published - 2009
Event	31st International Cosmic Ray Conference, ICRC 2009 - Lodz, Poland Duration: 7 Jul 2009 → 15 Jul 2009

Conference

Conference	31st International Cosmic Ray Conference, ICRC 2009
Country/Territory	Poland
City	Lodz
Period	7/07/09 → 15/07/09

Keywords

Solar cycle 24
Solar neutron telescopes
World-wide network

Cite this

Matsubara, Y., Muraki, Y., Sako, T., Itow, Y., Sakai, T., Shibata, S., Yuda, T., Ohnishi, M., Tsuchiya, H., Katayose, Y., Namikawa, K., Ogasawara, R., Mizumoto, Y., Kakimoto, F., Tsunesada, Y., Watanabe, K., Flückiger, E., Bütikofer, R., Chilingarian, A., ... Musalem, O. (2009). Status of the world-wide network of solar neutron telescopes in solar cycle 24. Paper presented at 31st International Cosmic Ray Conference, ICRC 2009, Lodz, Poland.

@conference{da214af7040140979d03037e1a54c2fa,

title = "Status of the world-wide network of solar neutron telescopes in solar cycle 24",

abstract = "A network of solar neutron telescopes has been developed since the middle of solar cycle 22. We have detected several important solar neutron events until the end of solar cycle 23 using solar neutron telescopes, but the accumulation of more solar neutron events is indispensable to eclucidate the acceleration mechanism of high energy particles. The data of the solar magnetic field with a space resolution of 0.3 arcsec obtained by Hinode satellite will be useful to understand solar neutron events more efficiently than during the previous solar cycles. In this paper we discuss the expected scientific results obtained by the world-wide network of solar neutron telescopes during solar cycle 24.",

keywords = "Solar cycle 24, Solar neutron telescopes, World-wide network",

author = "Y. Matsubara and Y. Muraki and T. Sako and Y. Itow and T. Sakai and S. Shibata and T. Yuda and M. Ohnishi and H. Tsuchiya and Y. Katayose and K. Namikawa and R. Ogasawara and Y. Mizumoto and F. Kakimoto and Y. Tsunesada and K. Watanabe and E. Fl{\"u}ckiger and R. B{\"u}tikofer and A. Chilingarian and G. Hovsepyan and Y. Tan and Zhang, {J. L.} and R. Ticona and W. Tavera and P. Miranda and J. Valdes-Galicia and Gonzalez, {L. X.} and A. Hurtado and O. Musalem",

year = "2009",

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

note = "31st International Cosmic Ray Conference, ICRC 2009 ; Conference date: 07-07-2009 Through 15-07-2009",

}

Matsubara, Y, Muraki, Y, Sako, T, Itow, Y, Sakai, T, Shibata, S, Yuda, T, Ohnishi, M, Tsuchiya, H, Katayose, Y, Namikawa, K, Ogasawara, R, Mizumoto, Y, Kakimoto, F, Tsunesada, Y, Watanabe, K, Flückiger, E, Bütikofer, R, Chilingarian, A, Hovsepyan, G, Tan, Y, Zhang, JL, Ticona, R, Tavera, W, Miranda, P, Valdes-Galicia, J, Gonzalez, LX, Hurtado, A & Musalem, O 2009, 'Status of the world-wide network of solar neutron telescopes in solar cycle 24', Paper presented at 31st International Cosmic Ray Conference, ICRC 2009, Lodz, Poland, 7/07/09 - 15/07/09.

TY - CONF

T1 - Status of the world-wide network of solar neutron telescopes in solar cycle 24

AU - Matsubara, Y.

AU - Muraki, Y.

AU - Sako, T.

AU - Itow, Y.

AU - Sakai, T.

AU - Shibata, S.

AU - Yuda, T.

AU - Ohnishi, M.

AU - Tsuchiya, H.

AU - Katayose, Y.

AU - Namikawa, K.

AU - Ogasawara, R.

AU - Mizumoto, Y.

AU - Kakimoto, F.

AU - Tsunesada, Y.

AU - Watanabe, K.

AU - Flückiger, E.

AU - Bütikofer, R.

AU - Chilingarian, A.

AU - Hovsepyan, G.

AU - Tan, Y.

AU - Zhang, J. L.

AU - Ticona, R.

AU - Tavera, W.

AU - Miranda, P.

AU - Valdes-Galicia, J.

AU - Gonzalez, L. X.

AU - Hurtado, A.

AU - Musalem, O.

PY - 2009

Y1 - 2009

N2 - A network of solar neutron telescopes has been developed since the middle of solar cycle 22. We have detected several important solar neutron events until the end of solar cycle 23 using solar neutron telescopes, but the accumulation of more solar neutron events is indispensable to eclucidate the acceleration mechanism of high energy particles. The data of the solar magnetic field with a space resolution of 0.3 arcsec obtained by Hinode satellite will be useful to understand solar neutron events more efficiently than during the previous solar cycles. In this paper we discuss the expected scientific results obtained by the world-wide network of solar neutron telescopes during solar cycle 24.

AB - A network of solar neutron telescopes has been developed since the middle of solar cycle 22. We have detected several important solar neutron events until the end of solar cycle 23 using solar neutron telescopes, but the accumulation of more solar neutron events is indispensable to eclucidate the acceleration mechanism of high energy particles. The data of the solar magnetic field with a space resolution of 0.3 arcsec obtained by Hinode satellite will be useful to understand solar neutron events more efficiently than during the previous solar cycles. In this paper we discuss the expected scientific results obtained by the world-wide network of solar neutron telescopes during solar cycle 24.

KW - Solar cycle 24

KW - Solar neutron telescopes

KW - World-wide network

UR - http://www.scopus.com/inward/record.url?scp=84899116885&partnerID=8YFLogxK

M3 - Artículo

AN - SCOPUS:84899116885

T2 - 31st International Cosmic Ray Conference, ICRC 2009

Y2 - 7 July 2009 through 15 July 2009

ER -

Status of the world-wide network of solar neutron telescopes in solar cycle 24

Abstract

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Keywords

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