Updated study on multi-TeV cosmic-ray modulation with the Tibet Ⅲ air shower array using the east-west method

BI Xiao-Jun; CHEN Tian-Lu; CHEN Wen-Yi

doi:10.1088/1674-1137/37/3/035001

Chinese Physics C> 2013, Vol. 37> Issue(3) : 035001 DOI: 10.1088/1674-1137/37/3/035001

Updated study on multi-TeV cosmic-ray modulation with the Tibet Ⅲ air shower array using the east-west method

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We study the sidereal and solar time modulation of multi-TeV cosmic rays using the east-west method with Tibet Ⅲ air shower array data taken from November 1999 to December 2008. The statistics are twice the amount used in our previous paper. In this analysis, the amplitude of the observed sidereal time modulation is about 0.1%, and the modulation shows an excess from about 4 to 7 hours and a deficit around 12 hours in local sidereal time. The sidereal time modulation has a weak dependence on the primary energy of the cosmic rays. However, the solar time modulation shows a large energy dependence. We find that the solar time modulation is fairly consistent with the prediction of the Compton-Getting effect for high-energy samples (6.2 TeV and 12.0 TeV), but exceeds the prediction for the low-energy sample (4.0 TeV). Such a discrepancy may be due to the solar modulation or the characteristics of the experimental device in the near threshold energy.

References

[1]

Nagashima K et al. Journal of Geophysical Research, 1998, 103: 17429-17440[2] Hall D L. Journal of Geophysical Research, 1998, 10: 367[3] Amenomori M et al. Science, 2006, 314: 439-442[4] Guillian G et al. Phys. Rev. D, 2007, 75: 062003[5] The Pierre Auger Collaboration. Science, 2007, 318: 938-943 [arXiv:astroph:0711.2256][6] The EAS-TOP Collaboration. 28th International Cosmic Ray Conference, 2003, 183-186[7] Erlykin A D, Wolfendale A W. Astropart. Phys, 2006, 25: 183[8] Compton A H, Getting I A. Phys. Rev, 1935, 47: 817[9] Krymsky G F. Geomagn. Aeron, 1964, 977: 763[10] Parker E N. Planet. Space. Sci., 1965, 13: 9[11] Amenomori M et al. AIP. Conf. Proc., 2010, 1302: 285-290[12] Munakata K et al. arXiv: axtroph/0811.0422[13] Munakata K et al. Phys. Rev. D, 1997, 56: 23[14] Ambrosio M et al. Phys. Rev. D, 2003, 67: 042002[15] Cutler D J, Groom D E. Nature, 1986, 322: 434[16] Amenomori M et al. Phys. Rev. Lett, 2004, 93: 061101[17] Amenomori M et al. The Astrophysical Journal, 2005, 626: 29-32[18] Amenomori M et al. Phys. Rev. Lett, 1992, 69: 2468[19] Amenomori M et al. 27th International Cosmic Ray Conference, 2001, 573

[1]	F. Aharonian , V. Alekseenko , Q. An , , L.X. Bai , Y.W. Bao , D. Bastieri , X.J. Bi , H. Cai , Zhe Cao , Zhen Cao , J. Chang , J.F. Chang , X.C. Chang , S.P. Chao , B.M. Chen , J. Chen , L. Chen , L. Chen , M.L. Chen , M.J. Chen , Q.H. Chen , S.H. Chen , S.Z. Chen , T.L. Chen , X.L. Chen , Y. Chen , N. Cheng , Y.D. Cheng , S.W. Cui , X.H. Cui , Y.D. Cui , B.Z. Dai , H.L. Dai , Z.G. Dai , , B. D'Ettorre Piazzoli , J. Fang , J.H. Fan , Y.Z. Fan , C.F Feng , L. Feng , S.H. Feng , Y.L. Feng , B. Gao , Q. Gao , W. Gao , M.M. Ge , L.S. Geng , G.H. Gong , Q.B. Gou , M.H. Gu , Y.Q. Guo , Y.Y. Guo , Y.A. Han , H.H. He , J.C. He , M. Heller , S.L. He , Y. He , C. Hou , D.H. Huang , Q.L. Huang , W.H. Huang , X.T. Huang , H.B. Hu , S. Hu , H.Y. Jia , K. Jiang , F. Ji , C. Jin , X.L. Ji , K. Levochkin , E.W. Liang , Y.F Liang , Cheng Li , Cong Li , F. Li , H. Li , H.B. Li , H.C. Li , H.M. Li , J. Li , K. Li , W.L. Li , X. Li , X.R. Li , Y. Li , Z. Li , Z. Li , B. Liu , C. Liu , D. Liu , H.D. Liu , H. Liu , J. Liu , J.Y. Liu , M.Y. Liu , R.Y. Liu , S.M. Liu , W. Liu , Y.N. Liu , Z.X. Liu , W.J. Long , R. Lu , H.K. Lv , B.Q. Ma , L.L. Ma , J.R. Mao , A. Masood , X.H. Ma , W. Mitthumsiri , T. Montaruli , Y.C. Nan , P. Pattarakijwanich , Z.Y. Pei , B.Q. Qiao , M.Y. Qi , D. Ruffolo , V. Rulev , A. Sáiz , L. Shao , O. Shchegolev , X.D. Sheng , J.R. Shi , Y. Stenkin , V. Stepanov , Z.B. Sun , P.H.T. Tam , Z.B. Tang , W.W. Tian , D.D. Volpe , C. Wang , H. Wang , H.G. Wang , J.C. Wang , L.Y. Wang , W. Wang , W. Wang , X.G. Wang , X.Y. Wang , X.J. Wang , Y.D. Wang , Y.J. Wang , Y.N. Wang , Y.P. Wang , Z. Wang , Z.H. Wang , Z.X. Wang , D.M. Wei , J.J. Wei , T. Wen , C.Y. Wu , H.R. Wu , S. Wu , W.X. Wu , X.F. Wu , G.M. Xiang , G. Xiao , G.G. Xin , Y. Xing , R.X. Xu , L. Xue , D.H. Yan , C.W. Yang , F.F. Yang , L.L. Yang , M.J. Yang , R.Z. Yang , S.B. Yang , Y.H. Yao , Z.G. Yao , Y.M. Ye , L.Q. Yin , N. Yin , X.H. You , Z.Y. You , Q. Yuan , Y.H. Yu , Z.J. Jiang , H.D. Zeng , T.X. Zeng , W. Zeng , Z.K. Zeng , M. Zha , B.B. Zhang , H.M. Zhang , H.Y. Zhang , J.L. Zhang , J.W. Zhang , L. Zhang , P.F. Zhang , P.P. Zhang , S.R. Zhang , S.S. Zhang , X. Zhang , X.P. Zhang , Yi Zhang , Yong Zhang , Y.F.g Zhang , B. Zhao , J. Zhao , L. Zhao , L.Z. Zhao , F. Zheng , Y. Zheng , J.N. Zhou , P. Zhou , R. Zhou , X.X. Zhou , C.G. Zhu , F.R. Zhu , H. Zhu , K.J. Zhu , X. Zuo , (LHAASO Collaboration) . Prospects for a multi-TeV gamma-ray sky survey with the LHAASO water Cherenkov detector array. Chinese Physics C, 2020, 44(6): 065001. doi: 10.1088/1674-1137/44/6/065001
[2]	Ran Ding , Zhi-Long Han , Li Huang , Yi Liao . Phenomenology of colored radiative neutrino mass model and its implications on cosmic-ray observations. Chinese Physics C, 2018, 42(10): 103101. doi: 10.1088/1674-1137/42/10/103101
[3]	Xun-Xiu Zhou , Lan-Lan Gao , Yu Zhang , Yi-Qing Guo , Qing-Qi Zhu , Huan-Yu Jia , Dai-Hui Huang . Sensitivity study of (10,100) GeV gamma-ray bursts with double shower front events from ARGO-YBJ. Chinese Physics C, 2016, 40(7): 075001. doi: 10.1088/1674-1137/40/7/075001
[4]	Yong-ji Xie , Zhong-hua Qin , Xiao-yan Ma , Jian Zhang , Ling-hui Wu , Wan Xie , Ming-yi Dong , Jing Dong , Xiao-lu Ji , Xiao-shan Jiang , Qun Ou-yang , Ke-jun Zhu , Yuan-bo Chen . Construction and cosmic-ray test of the new inner drift chamber for BESIII. Chinese Physics C, 2016, 40(9): 096003. doi: 10.1088/1674-1137/40/9/096003
[5]	FENG Yu , GONG Bin , WAN Lu-Ping , WANG Jian-Xiong . An updated study of Y production and polarizationat the Tevatron and LHC. Chinese Physics C, 2015, 39(12): 123102. doi: 10.1088/1674-1137/39/12/123102
[6]	ZHANG Fei , FAN Rui-Rui , PENG Wen-Xi , DONG Yi-Fan , GONG Ke , LIANG Xiao-Hua , LIU Ya-Qing , WANG Huan-Yu . A prototype silicon detector system for space cosmic-ray charge measurement. Chinese Physics C, 2014, 38(6): 066101. doi: 10.1088/1674-1137/38/6/066101
[7]	LIU Cheng , BI Xiao-Jun , CHEN Tian-Lu . Performance of the muon detector A under TIBET Ⅲ array. Chinese Physics C, 2013, 37(2): 026001. doi: 10.1088/1674-1137/37/2/026001
[8]	GE Yong-Shuai , WANG Zhi-Gang , YU Bo-Xiang , XIE Yu-Guang , ZHANG Ai-Wu , XUE Zhen , LIU Ying-Biao , GAO Long , NIU Shun-Li , CAI Xiao , FANG Jian , SUN Xi-Lei , NING Fei-Peng , ZHOU Li , HU Tao , , . A novel 2-dimensional cosmic ray position detector based on a CsI(Na) pixel array and an ICCD camera. Chinese Physics C, 2012, 36(11): 1101-1105. doi: 10.1088/1674-1137/36/11/011
[9]	FENG Zhao-Yang , ZHANG Yi , LIU Cheng , FAN Chao , LI Hong-Chao , WANG Bo , WU Han-Rong , HU Hong-Bo , LU Hong , TAN You-Heng . Study on the separation of 100 TeV γ-rays from cosmic rays for the Tibet ASγ experiment. Chinese Physics C, 2011, 35(2): 153-157. doi: 10.1088/1674-1137/35/2/009
[10]	WU Zhi , LIU Jian-Bei , QIN Zhong-Hua , WU Ling-Hui , CHEN Chang , CHEN Yuan-Bo , CHEN Ma-Li , CHEN Xi-Hui , DONG Ming-Yi , GUAN Bei-Ju , HUANG Jie , JIANG Xiao-Shan , JIN Yan , LI Fei , LI Ren-Ying , LI Xiao-Nan , LEI Guang-Kun , LIU Rong-Guang , LUO Xiao-Lan , MA Xiao-Yan , SHENG Hua-Yi , SUN Han-Sheng , TANG Xiao , WANG Lan , WANG Liang , XU Mei-Hang , ZHANG Jian , ZHANG Hong-Yu , ZHANG Yin-Hong , ZHAO Yu-Bin , ZHAO Ping-Ping , ZHU Ke-Jun , ZHU Qi-Ming , ZHUANG Bao-An . Tuning of the cosmic-ray test system of the BESⅢ drift chamber. Chinese Physics C, 2010, 34(7): 983-987. doi: 10.1088/1674-1137/34/7/010
[11]	CAO Zhen (for the LHAASO collaboration) . A future project at tibet: the large high altitude air shower observatory (LHAASO). Chinese Physics C, 2010, 34(2): 249-252. doi: 10.1088/1674-1137/34/2/018
[12]	LIANG Yu-Tie , MAO Ya-Jun , YOU Zheng-Yun . Study of BESⅢ MUC offline software with cosmic-ray data. Chinese Physics C, 2009, 33(7): 562-566. doi: 10.1088/1674-1137/33/7/011
[13]	WANG Yue , BI Xiao-Jun , CUI Shu-Wang , DING Lin-Kai . An updated search of steady TeV γ-ray point sources in northern hemisphere using the Tibet air shower array. Chinese Physics C, 2008, 32(11): 868-872. doi: 10.1088/1674-1137/32/11/004
[14]	ZHANG Ji-Long , CUI Shu-Wang , DING Lin-Kai , DING Xiao-Hong , FENG Cun-Feng , FENG Zhen-Yong , GAO Xiao-Yu , GENG Qing-Xi , GUO Hong-Wei , HE Hui-Hai , HE Mao , , , , , , . Search for a TeV Gamma Rays Emission from the Shell-like SNP G40.5-0.5 Using the Yangbajing Extend Air Shower Array. Chinese Physics C, 2006, 30(1): 13-17.
[15]	JIA Huan-Yu , WANG Shun-Jin . Study of the Time Variation of 10TeV Cosmic Ray. Chinese Physics C, 2001, 25(4): 277-282.
[16]	XU XianWu , DING LinKai , CAO PeiYuan , DAI BenZhong , FENG ZhenYong , FU Yu , GUO HongWei , HE Mao , HUANG Qing , HUO AnXiang , JIA HuanYu , LI JinYu , LIU ShaoMin , , , , . Search for TeV Gamma Rays from the Crab Nebula with Tibet Ⅱ/HD AS Array. Chinese Physics C, 2000, 24(6): 473-477.
[17]	Liu Shaomin , Ding Linkai , Shi Ce , Zhaxiciren , Zhaxisanzhu , Mu Jun , Wnag Hui , Lu Hong , Feng Zhenyong , Ren Jingru , Yu Guangce , Zhou Wende , Labaciren , Meng Xianru , Meng Lie , Zhang Jilong , Zhang Chunsheng , Zhang Huimin , Shi Zhizheng , Jia Huanyiu , Mei Dongming , Huang Qing , Tan Youheng , Huo Anxiang , Dai Benzhong . Correlation Between Sun Shadows of 10 TeV Cosmic Ray and the Solar Activity. Chinese Physics C, 1997, 21(S4): 11-18.
[18]	Ding Linkai , Dai Benzhong , Feng Zhenyong , Huang Qing , Huo Anxiang , Jia Huanyu , Labaciren , Mei Dongming , Meng Lie , Meng Xianru , Mu Jun , Ren Jingru , Shi Zhizheng , Tan Youheng , Wang Hui , Yu Guangce , Zhaxiciren , Zhaxisanzhu , Zhou Wende , Zhang Chunsheng , Zhang Huimin . Search for 10 TeV Gamma-Ray Bursts with the Tibet Air Shower Array. Chinese Physics C, 1997, 21(S3): 9-16.
[19]	Luo Guangxuan , Tan Youheng , Zhang Chunsheng , Dong Yuju , Yuan Peng , Zhang Huimin , Wang Hui , Yuang Yukui , Li Jing . Energy Spectrum of Primary Cosmic Rays at the “Knee” Region Observed with the Huairou Air Shower Array. Chinese Physics C, 1995, 19(S4): 325-331.
[20]	Jia Huanyu , Cao Zhen , Zhang Huimin . Meteorological Effects on the Trigger Rate of Air Showers Observed with the Tibet Air Shower Array. Chinese Physics C, 1994, 18(S3): 235-242.

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BI Xiao-Jun, CHEN Tian-Lu and CHEN Wen-Yi. Updated study on multi-TeV cosmic-ray modulation with the Tibet Ⅲ air shower array using the east-west method[J]. Chinese Physics C, 2013, 37(3): 035001. doi: 10.1088/1674-1137/37/3/035001

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Received: 2012-05-09
Revised: 2012-05-28

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沈阳化工大学材料科学与工程学院沈阳 110142

Updated study on multi-TeV cosmic-ray modulation with the Tibet Ⅲ air shower array using the east-west method

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Updated study on multi-TeV cosmic-ray modulation with the Tibet Ⅲ air shower array using the east-west method

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