W
W. Y. Chen
Researcher at Chinese Academy of Sciences
Publications - 24
Citations - 350
W. Y. Chen is an academic researcher from Chinese Academy of Sciences. The author has contributed to research in topics: Cosmic ray & Air shower. The author has an hindex of 7, co-authored 24 publications receiving 189 citations.
Papers
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Journal ArticleDOI
First Detection of sub-PeV Diffuse Gamma Rays from the Galactic Disk: Evidence for Ubiquitous Galactic Cosmic Rays beyond PeV Energies.
M. Amenomori,Yongjun Bao,X. J. Bi,Donghong Chen,T. L. Chen,W. Y. Chen,Xu Chen,Yu-Lei Chen,Cirennima,S. W. Cui,Danzengluobu,L. K. Ding,J. Fang,K. Fang,C. F. Feng,Zhaoyang Feng,Z. Y. Feng,Qi Gao,Q. B. Gou,Y. Q. Guo,Yang Guo,H. H. He,Z. T. He,K. Hibino,N. Hotta,Haibing Hu,H. B. Hu,Jian Huang,H. Y. Jia,L. L. Jiang,H. B. Jin,Katsuaki Kasahara,Y. Katayose,Chihiro Kato,Shigeaki Kato,K. Kawata,W. Kihara,Y. Ko,Masayoshi Kozai,Labaciren,Gui-Ming Le,Ang Li,Ang Li,H. J. Li,W. J. Li,W. J. Li,Y. H. Lin,B. Liu,C. X. Liu,J. S. Liu,Minghui Liu,Wenwei Liu,Y. Q. Lou,Hong-peng Lu,X. R. Meng,Kazuoki Munakata,H. Nakada,Y. Nakamura,H. Nanjo,Masaki Nishizawa,M. Ohnishi,T. Ohura,S. Ozawa,X. L. Qian,X. B. Qu,To. Saito,M. Sakata,Takashi Sako,J. Shao,J. Shao,M. Shibata,A. Shiomi,H. Sugimoto,W. Takano,Masato Takita,Y. H. Tan,N. Tateyama,Shoji Torii,Harufumi Tsuchiya,S. Udo,Huaguang Wang,H. R. Wu,L. Xue,Y. Yamamoto,Zicai Yang,Y. Yokoe,A. F. Yuan,L. M. Zhai,H. M. Zhang,Jia Zhang,Xiang Zhang,X. Y. Zhang,Y. Zhang,Yi Zhang,Ying Zhang,Shi-Ping Zhao,Zhaxisangzhu,X. X. Zhou,mrow> γ<,mrow,msub +100 more
TL;DR: For the first time, the long-awaited detection of diffuse gamma rays with energies between 100 TeV and 1 PeV in the Galactic disk was reported in this paper, which is consistent with expectations from the hadronic emission scenario in which gamma rays originate from the decay of π 0's produced through the interaction of protons with the interstellar medium.
Journal ArticleDOI
Concept Design of the "Guanlan" Science Mission: China's Novel Contribution to Space Oceanography
Ge Chen,Junwu Tang,Chaofang Zhao,Songhua Wu,Fangjie Yu,Chunyong Ma,Yongsheng Xu,W. Y. Chen,Yunhua Zhang,Jie Liu,Lixin Wu +10 more
TL;DR: In this paper, a dual-frequency (Ku and Ka) interferometric altimetry (IA) and a near-nadir pointing ocean lidar (OL) was used to resolve the ocean variability at submeso and sub-week scales with a centimeter-level accuracy, while also partially revealing marine life systems and ecosystems.
Journal ArticleDOI
Probe of the Solar Magnetic Field Using the “Cosmic-Ray Shadow” of the Sun
M. Amenomori,X. J. Bi,Donghong Chen,T. L. Chen,W. Y. Chen,S. W. Cui,Danzengluobu,L. K. Ding,C. F. Feng,Zhaoyang Feng,Zhenyong Feng,Q. B. Gou,Y. Q. Guo,K. Hakamada,Huihai He,Z. T. He,K. Hibino,N. Hotta,Haibing Hu,H. B. Hu,Jing Huang,H. Y. Jia,L. L. Jiang,F. Kajino,K. Kasahara,Y. Katayose,Chihiro Kato,Kazumasa Kawata,Labaciren,Gui-Ming Le,A. F. Li,A. F. Li,Haifeng Li,W. J. Li,C. X. Liu,J. S. Liu,Minghui Liu,Hsiao-Chi Lu,X. R. Meng,K. Mizutani,Kazuoki Munakata,H. Nanjo,Masaki Nishizawa,M. Ohnishi,I. Ohta,H. Onuma,Shunsuke Ozawa,X. L. Qian,X. B. Qu,Takeshi Saito,Takashi Saito,M. Sakata,T. K. Sako,J. Shao,M. Shibata,A. Shiomi,T. Shirai,H. Sugimoto,Masato Takita,Y. H. Tan,N. Tateyama,Shoji Torii,Harufumi Tsuchiya,S. Udo,Huaguang Wang,H. R. Wu,L. Xue,Y. Yamamoto,Zicai Yang,S. Yasue,A. F. Yuan,T. Yuda,L. M. Zhai,H. M. Zhang,Jia Zhang,X. Y. Zhang,Y. Zhang,Yi Zhang,Ying Zhang,Zhaxisangzhu,X. X. Zhou +80 more
TL;DR: This is the first successful attempt to evaluate the coronal magnetic field models by using the Sun's shadow observed in the TeV cosmic-ray flux, and it is found that the intensity deficit in the simulated Sun’s shadow is very sensitive to the corona magnetic field structure.
Journal ArticleDOI
Potential PeVatron supernova remnant G106.3+2.7 seen in the highest-energy gamma rays
M. Amenomori,Yongjun Bao,X. J. Bi,Donghong Chen,T. L. Chen,W. Y. Chen,Xu Chen,Yu-Lei Chen,Cirennima,S. W. Cui,Danzengluobu,L. K. Ding,J. Fang,Kun Fang,C. F. Feng,Zhaoyang Feng,Z. Y. Feng,Qi Gao,Q. B. Gou,Y. Q. Guo,Yang Guo,H. H. He,Z. T. He,K. Hibino,N. Hotta,Haibing Hu,H. B. Hu,Jian Huang,H. Y. Jia,L. L. Jiang,H. B. Jin,K. Kasahara,Y. Katayose,Chihiro Kato,Shigeaki Kato,K. Kawata,W. Kihara,Y. Ko,Masayoshi Kozai,Labaciren,Gui-Ming Le,Ang Li,H. J. Li,W. J. Li,Y. H. Lin,B. Liu,C. X. Liu,J. S. Liu,Minghui Liu,Wenwei Liu,Y. Q. Lou,Hsiao-Chi Lu,X. R. Meng,Kazuoki Munakata,H. Nakada,Y. Nakamura,H. Nanjo,Masaki Nishizawa,M. Ohnishi,T. Ohura,S. Ozawa,X. L. Qian,X. B. Qu,Takeshi Saito,M. Sakata,T. K. Sako,J. Shao,M. Shibata,A. Shiomi,H. Sugimoto,W. Takano,M. Takita,Y. H. Tan,N. Tateyama,S. Torii,Harufumi Tsuchiya,S. Udo,Huaguang Wang,H. R. Wu,L. Xue,Y. Yamamoto,Zicai Yang,Y. Yokoe,A. F. Yuan,L. M. Zhai,H. M. Zhang,Jia Zhang,X. Y. Zhang,Xuan Zhang,Y. Zhang,Yi Zhang,Ying Zhang,Shi-Ping Zhao,Zhaxisangzhu,X. X. Zhou +94 more
TL;DR: In this article, the gamma-ray emission from the supernova remnant G106.3+2.7 above 10 teraelectronvolts (TeV) has been observed and it was shown that the very high-energy gamma ray emission above 10 TeV is well correlated with a molecular cloud rather than the pulsar PSR J2229+6114.
Journal ArticleDOI
Potential PeVatron supernova remnant G106.3+2.7 seen in the highest-energy gamma rays
M. Amenomori,Yongjun Bao,X. J. Bi,Donghong Chen,T. L. Chen,W. Y. Chen,Xu Chen,Yu-Lei Chen,Cirennima, Cui, S. W.,Danzengluobu, Ding, L. K.,J. Fang,Kun Fang,C. F. Feng,Zhaoyang Feng,Z. Y. Feng,Qi Gao,Q. B. Gou,Y. Q. Guo,Yang Guo,H. H. He,Z. T. He,K. Hibino,N. Hotta,Haibing Hu,H. B. Hu,Jian Huang,H. Y. Jia,L. L. Jiang,H. B. Jin,K. Kasahara,Y. Katayose,Chihiro Kato,Shigeaki Kato,K. Kawata,W. Kihara,Y. Ko,Masayoshi Kozai,Labaciren, Le, G. M.,Ang Li,H. J. Li,W. J. Li,Y. H. Lin,B. Liu,C. X. Liu,J. S. Liu,Minghui Liu,Wenwei Liu,Y. Q. Lou,Hsiao-Chi Lu,X. R. Meng,Kazuoki Munakata,H. Nakada,Y. Nakamura,H. Nanjo,Masaki Nishizawa,M. Ohnishi,T. Ohura,S. Ozawa,X. L. Qian,X. B. Qu,Takeshi Saito,M. Sakata,T. K. Sako,J. Shao,M. Shibata,A. Shiomi,H. Sugimoto,W. Takano,M. Takita,Y. H. Tan,N. Tateyama,S. Torii,Harufumi Tsuchiya,S. Udo,Huaguang Wang,H. R. Wu,L. Xue,Y. Yamamoto,Zicai Yang,Y. Yokoe,A. F. Yuan,L. M. Zhai,H. M. Zhang,Jia Zhang,X. Y. Zhang,Xuan Zhang,Y. Zhang,Yi Zhang,Ying Zhang,Shi-Ping Zhao,Zhaxisangzhu, Zhou, X. X. +90 more
TL;DR: In this paper, the gamma-ray emission from the supernova remnant G106.3+2.7 above 10 teraelectronvolts (TeV) was observed and it was shown that the very high-energy gamma ray emission above 10 TeV is well correlated with a molecular cloud rather than the pulsar PSR J2229+6114.