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Search for the solar neutrons using the Yangbajing neutron monitor and the neutron telescope during the 23rd solar cycle

Zhang, J. L. and Tan, Y. H. and Lu, H. and Wang, H. and Tsuchiya, H. and Matsuoka, M. and Yamada, Y. and Yuda, T. and Muraki, Y. and Miyasaka, H. (2005) Search for the solar neutrons using the Yangbajing neutron monitor and the neutron telescope during the 23rd solar cycle. In: Proceedings of the 29th International Cosmic Ray Conference. Vol.1. Tata Institute of Fundamental Research , Pune, India, pp. 9-12. https://resolver.caltech.edu/CaltechAUTHORS:20150401-095718304

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Abstract

The geographical location of Yangbajing (latitude 30, 4300m above sea level) has advantages for the direct detection of the solar are neutron events. The Yangbajing neutron monitor and neutron telescope were established in 1998 October at Yangbajing under the China-Japan cooperation and be used for the observation of solar neutron events during the 23th solar cycle. On 28 November 1998 the Yangbajing neutron monitor recorded a 3.8 sigma excess that has time coincidence with the reported neutron event of the Yangbajing neutron telescope. The response of Yangbajing neutron monitor and neutron telescope on the solar particle event associated with theX17.2 class are at October 28, 2003 was researched too.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://adsabs.harvard.edu/abs/2005ICRC....1....9ZADSArticle
Group:Space Radiation Laboratory
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Space Radiation Laboratory2005-32
Record Number:CaltechAUTHORS:20150401-095718304
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20150401-095718304
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:56274
Collection:CaltechAUTHORS
Deposited By: Deborah Miles
Deposited On:22 Apr 2015 01:14
Last Modified:03 Oct 2019 08:12

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