Zobrazeno 1 - 10
of 47
pro vyhledávání: '"Chang-Chun Ning"'
Autor:
M. Iacovacci, L. L. Ma, X. H. Ma, Hongbo Hu, X. Y. Zhang, Minghui Liu, L. Perrone, Zihuang Cao, P. Creti, Haifeng Li, R. Santonico, Yicheng Guo, J. B. Zhao, P. Salvini, A. Budano, Chang-Chun Ning, Cunfeng Feng, Zhaoyang Feng, Fudong Shi, Z. G. Yao, C. Y. Wu, B. D'Ettorre Piazzoli, H. Lu, F. R. Zhu, S. Mastroianni, Danzengluobu, G. Di Sciascio, I. De Mitri, S. M. Mari, X. C. Yang, Piero Vallania, T. L. Chen, Zhaxiciren, G. Liguori, L. Xue, Paolo Camarri, Zhenyong Feng, B. Bartoli, C. X. Liu, H. W. Wang, Zhaxisangzhu, J. K. K. Liu, H. Y. Jia, Longzhou Zhang, Q. Q. Zhu, M. Zha, X. J. Bi, M. Panareo, G. Mancarella, S. W. Cui, S. Z. Chen, T. Di Girolamo, H. R. Wu, B. Z. Dai, F. Ruggieri, P. Branchini, Q. B. Gou, A. F. Yuan, Labaciren, Q. Y. Yang, G. Zizzi, H. H. He, Y. H. Tan, A. D'Amone, X. D. Sheng, Paolo Bernardini, Paolo Montini, R. Iuppa, R. Cardarelli, G. Marsella, S. Vernetto, Pengnian Shen, S. Catalanotti, P. Pistilli, H. M. Zhang, X. X. Zhou, A. Surdo, Carlo Vigorito, Haibing Hu, Y. Zhang, D. Martello
Resistive Plate Chambers have largely been used in High Energy Physics and Cosmic Ray research. In view of using this detector for calorimetry applications it is important to know the maximum measurable particle density, or its intrinsic linearity li
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3342122fd8d3b000db59b33e0ecbc21f
http://hdl.handle.net/10447/547024
http://hdl.handle.net/10447/547024
Akademický článek
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Autor:
X. C. Yang, H. H. He, T. Di Girolamo, Zhenyong Feng, H. Y. Jia, B. D'Ettorre Piazzoli, L. Xue, Hong-peng Lu, P. Pistilli, H. M. Zhang, X. X. Zhou, M. Iacovacci, M. Zha, Labaciren, X. D. Sheng, S. M. Mari, J. K. K. Liu, A. Surdo, Paolo Bernardini, L. L. Ma, Haibing Hu, Longzhou Zhang, H. W. Wang, J. B. Zhao, P. Salvini, Chang-Chun Ning, C. X. Liu, H. J. Li, H. R. Wu, Zhaoyang Feng, G. Marsella, X. J. Bi, Y. Zhang, Z. G. Yao, G. Mancarella, Zhaxisangzhu, C. Y. Wu, B. Bartoli, S. Z. Chen, L. Perrone, R. Santonico, G. Di Sciascio, Y. H. Tan, Fudong Shi, B. Z. Dai, S. Mastroianni, Carlo Vigorito, Zhaxiciren, F. R. Zhu, Danzengluobu, Y. Q. Guo, Q. Q. Zhu, I. De Mitri, Q. B. Gou, Zihuang Cao, Piero Vallania, T. L. Chen, A. F. Yuan, Pengnian Shen, S. Catalanotti, S. W. Cui, Hongbo Hu, C. F. Feng, P. Montini, X. H. Ma, X. Y. Zhang, Minghui Liu, R. Iuppa, S. Vernetto, A. D'Amone, Q. Y. Yang
Publikováno v:
Astroparticle Physics. 90:20-27
In 2011 ARGO-YBJ experiment has reported a work to study the absolute rigidity scale of the primary cosmic ray particles based on the Moon's shadow observation. Given the progress in high energy hadronic interaction models with LHC data, in cosmic ra
Autor:
CHANG,CHUN-NING, 張鈞甯
107
Culture not only affects the social value of a country, but also has a certain degree of influence on the business operations and decision-making. In different industries, due to different environmental factors and risks, enterprises therefo
Culture not only affects the social value of a country, but also has a certain degree of influence on the business operations and decision-making. In different industries, due to different environmental factors and risks, enterprises therefo
Externí odkaz:
http://ndltd.ncl.edu.tw/handle/hnn2e8
Autor:
Jin-Long Xu, Si-Ju Zhang, Guoyin Zhang, Bing-Gang Ju, Chuan-Peng Zhang, Chang-Chun Ning, Ye Xu, Naiping Yu, Jinghua Yuan, Annie Zavagno, Xiao-Lan Liu
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 627, pp.A27. ⟨10.1051/0004-6361/201935024⟩
Astronomy and Astrophysics-A&A, 2019, 627, pp.A27. ⟨10.1051/0004-6361/201935024⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 627, pp.A27. ⟨10.1051/0004-6361/201935024⟩
Astronomy and Astrophysics-A&A, 2019, 627, pp.A27. ⟨10.1051/0004-6361/201935024⟩
We aim to investigate the impact of the ionized radiation from the M16 HII region on the surrounding molecular cloud and on its hosted star formation. To present comprehensive multi-wavelength observations towards the M16 HII region, we used new CO d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::78d89a6026938a3de400de6c7280821b
Autor:
Xiao-Lan Liu, Jürgen Stutzki, Chang-Chun Ning, Karl Jacobs, Urs U. Graf, Chuan-Peng Zhang, Jun-Jie Wang, Nan Li, Gang Xu, Sheng-Li Qin, Qi Wu, Junzhi Wang, Naiping Yu, Jin-Long Xu, Yang Chen, Marc L. Miller, X. Guan, Danzengluobu, Jian-Bin Li, Tian-Lu Chen, Yuefang Wu, Guoyin Zhang
Publikováno v:
Research in Astronomy and Astrophysics. 19:183
We have performed a multi-wavelength study toward a quasi-sinusoidal filament (CFG028.68–0.28). A new large-scale 12CO J = 3 – 2 map was obtained from the China-Cologne Observation for SubMillimeter Astronomy (CCOSMA) 3m radio telescope. Based on
Autor:
Chun-ming Liu, Chang-chun Ning
Publikováno v:
DEStech Transactions on Social Science, Education and Human Science.
The distribution of routine performance score (RPC) and test score is investigated. It is found that most of students can get top RPC score. However, a lot of students fail in test. There is a distinct difference in the distribution of RPC and test s
Autor:
Bing-Gang Ju, Xiao-Lan Liu, Chuan-Peng Zhang, Ye Xu, Jin-Long Xu, Chang-Chun Ning, Naiping Yu
We performed a multi-wavelength study toward the filamentary cloud G47.06+0.26 to investigate the gas kinematics and star formation. We present the 12CO (J=1-0), 13CO (J=1-0) and C18O (J=1-0) observations of G47.06+0.26 obtained with the Purple Mount
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2234e575d69b49f8479f4d0bfec01d01
In this work, we perform a statistical investigation towards 50 high-mass clumps using the data from the Bolocam Galactic Plane Survey (BGPS) and the Millimetre Astronomy Legacy Team 90-GHz survey (MALT90). Eleven dense molecular lines (N$_2$H$^+$(1-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3cd442b3bb668b7d86381cb380cc96c5
Publikováno v:
Research in Astronomy and Astrophysics. 14:47-65
We have investigated 25 H II regions with bubble morphology in 13CO(1-0) and infrared data, to search the quantitative evidence for the triggering star formation by collect and collapse (CC) and radiatively driven implosion (RDI) models. These H II r