Crashworthiness Analysis and Evaluation of Fuselage Section with Sub-floor Composite Sinusoidal Specimens von Mou, H.L., Zou, T.C., Feng, Z.Y., Xie, J.

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Effects of irrigation regime and rice variety on greenhouse gas emissions and grain yields from paddy fields in central China von Feng, Z.Y., Qin, T., Du, X.Z., Sheng, F., Li, C.F.

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Multi-aspect size effect transition from micro to macroscale: Modelling and experiment von Feng, Z.Y., Li, H., Zhang, D., Guo, X.X., Chen, Y.Q., Fu, M.W.

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Cartilaginous endplate avulsion is associated with modic changes and endplate defects, and residual back and leg pain following lumbar discectomy von Feng, Z.Y., Hu, X.J., Zheng, Q.Q., Battié, M.C., Chen, Z., Wang, Y.

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Thermo-magnetic stability of magnetic Fe 3 O 4 nanoparticles for hyperthermia von Pan, Y.M., Zhang, W., Hu, Z.F., Feng, Z.Y., Zhang, X.P.

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Synchrotron radiation-based multi-analytical approach for studying underglaze color: The microstructure of Chinese Qinghua blue decors (Ming dynasty) von Wang, T., Zhu, T.Q., Feng, Z.Y., Fayard, B., Pouyet, E., Cotte, M., De Nolf, W., Salomé, M., Sciau, Ph

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Observation of Gamma Rays up to 320 TeV from the Middle-aged TeV Pulsar Wind Nebula HESS J1849-000 von Amenomori, M, Asano, S, Bao, Y.W, Bi, X.J, Chen, D, Chen, T.L, Chen, W.Y, Chen, Xu, Chen, Y, Cui, S.W, Ding, L.K, Fang, J.H, Fang, K, Feng, C.F, Feng, Zhaoyang, Feng, Z.Y, Gao, Qi, Gomi, A, Gou, Q.B, Guo, Y.Q, Guo, Y.Y, Hayashi, Y, He, H.H, He, Z.T, Hibino, K, Hotta, N, Hu, Haibing, Hu, H.B, Hu, K.Y, Huang, J, Jia, H.Y, Jiang, L, Jiang, P, Jin, H.B, Kasahara, K, Katayose, Y, Kato, C, Kato, S, Kawahara, I, Kawashima, T, Kawata, K, Kozai, M, Kurashige, D, Le, G.M, Li, A.F, Li, H.J, Li, W.J, Li, Y, Lin, Y.H, Liu, B, Liu, C, Liu, J.S, Liu, L.Y, Liu, M.Y, Liu, W, Lu, H, Meng, X.R, Meng, Y, Munakata, K, Nagaya, K, Nakamura, Y, Nakazawa, Y, Nanjo, H, Ning, C.C, Nishizawa, M, Noguchi, R, Ohnishi, M, Okukawa, S, Ozawa, S, Qian, X, Qian, X.L, Qu, X.B, Saito, T, Sakakibara, Y, Sakata, M, Sako, T, Sako, T.K, Sasaki, T, Shao, J, Shibata, M, Shiomi, A, Sugimoto, H, Takano, W, Takita, M, Tan, Y.H, Tateyama, N, Torii, S, Tsuchiya, H, Udo, S, Wang, H, Wang, S.F, Wang, Y.P, Wu, H.R, Wu, Q, Xu, J.L, Xue, L, Yang, Z, Yao, Y.Q, Yin, J, Yokoe, Y

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Anisotropy and Corotation of Galactic Cosmic Rays von Amenomori, M, Ayabe, S, Bi, X.J, Chen, D, Cui, S.W, Danzengluobu, Ding, L.K, Ding, X.H, Feng, C.F, Feng, Zhaoyang, Feng, Z.Y, Gao, X.Y, Geng, Q.X, Guo, H.W, He, H.H, He, M, Hibino, K, Hotta, N, Hu, Haibing, Hu, H.B, Huang, J, Huang, Q, Jia, H.Y, Kajino, F, Kasahara, K, Katayose, Y, Kato, C, Kawata, K, Labaciren, Le, G.M, Li, A.F, Li, J.Y, Lou, Y.-Q, Lu, H, Lu, S.L, Meng, X.R, Mizutani, K, Mu, J, Munakata, K, Nagai, A, Nanjo, H, Nishizawa, M, Ohnishi, M, Ohta, I, Onuma, H, Ouchi, T, Ozawa, S, Ren, J.R, Saito, T, Saito, T.Y, Sakata, M, Sako, T.K, Sasaki, T, Shibata, M, Shiomi, A, Shirai, T, Sugimoto, H, Takita, M, Tan, Y.H, Tateyama, N, Torii, S, Tsuchiya, H, Udo, S, Wang, B, Wang, H, Wang, X, Wang, Y.G, Wu, H.R, Xue, L, Yamamoto, Y, Yan, C.T, Yang, X.C, Yasue, S, Ye, Z.H, Yu, G.C, Yuan, A.F, Yuda, T, Zhang, H.M, Zhang, J.L, Zhang, N.J, Zhang, X.Y, Zhang, Y, Zhang, Yi, Zhaxisangzhu, Zhou, X.X

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Theoretical studies on the structural, electronic and optical properties of BeZnO alloys von Xiong, D.P., Zhou, S.L., He, M., Wang, Q., Zhang, W., Feng, Z.Y.

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Thermo-magnetic stability of magnetic Fe3O4 nanoparticles for hyperthermia von Pan, Y.M., Zhang, W., Hu, Z.F., Feng, Z.Y., Zhang, X.P.

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Ferroelectric and ferromagnetic properties of SrTi0.9Fe0.1O3−δ thin films von Wang, Y.G., Tang, X.G., Liu, Q.X., Jiang, Y.P., Feng, Z.Y.

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Outage probability minimising joint channel and power allocation for cognitive radio networks von XU, D, FENG, Z. Y, LIU, Y, ZHANG, P

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Are protons still dominant at the knee of the cosmic-ray energy spectrum? von Amenomori, M., Ayabe, S., Chen, D., Cui, S.W., Danzengluobu, Ding, L.K., Ding, X.H., Feng, C.F., Feng, Z.Y., Gao, X.Y., Geng, Q.X., Guo, H.W., He, H.H., He, M., Hibino, K., Hotta, N., Hu, Haibing, Hu, H.B., Huang, J., Huang, Q., Jia, H.Y., Kajino, F., Kasahara, K., Katayose, Y., Kato, C., Kawata, K., Labaciren, Le, G.M., Li, J.Y., Lu, H., Lu, S.L., Meng, X.R., Mizutani, K., Mu, J., Munakata, K., Nagai, A., Nanjo, H., Nishizawa, M., Ohnishi, M., Ohta, I., Onuma, H., Ouchi, T., Ozawa, S., Ren, J.R., Saito, T., Sakata, M., Sasaki, T., Shibata, M., Shiomi, A., Shirai, T., Sugimoto, H., Takita, M., Tan, Y.H., Tateyama, N., Torii, S., Tsuchiya, H., Udo, S., Wang, H., Wang, X., Wang, Y.G., Wu, H.R., Xue, L., Yamamoto, Y., Yan, C.T., Yang, X.C., Yasue, S., Ye, Z.H., Yu, G.C., Yuan, A.F., Yuda, T., Zhang, H.M., Zhang, J.L., Zhang, N.J., Zhang, X.Y., Zhang, Y., Zhang, Yi, Zhaxisangzhu, Zhou, X.X.

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Cosmic-ray energy spectrum around the knee obtained by the Tibet experiment and future prospects von Amenomori, M., Bi, X.J., Chen, D., Cui, S.W., Danzengluobu, Ding, L.K., Ding, X.H., Fan, C., Feng, C.F., Feng, Zhaoyang, Feng, Z.Y., Gao, X.Y., Geng, Q.X., Guo, H.W., He, H.H., He, M., Hibino, K., Hotta, N., Hu, Haibing, Hu, H.B., Huang, J., Huang, Q., Jia, H.Y., Kajino, F., Kasahara, K., Katayose, Y., Kato, C., Kawata, K., Labaciren, Le, G.M., Li, A.F., Li, J.Y., Lou, Y.-Q., Lu, H., Lu, S.L., Meng, X.R., Mizutani, K., Mu, J., Munakata, K., Nagai, A., Nanjo, H., Nishizawa, M., Ohnishi, M., Ohta, I., Onuma, H., Ouchi, T., Ozawa, S., Ren, J.R., Saito, T., Saito, T.Y., Sakata, M., Sako, T.K., Shibata, M., Shiomi, A., Shirai, T., Sugimoto, H., Takita, M., Tan, Y.H., Tateyama, N., Torii, S., Tsuchiya, H., Udo, S., Wang, B., Wang, H., Wang, X., Wang, Y., Wang, Y.G., Wu, H.R., Xue, L., Yamamoto, Y., Yan, C.T., Yang, X.C., Yasue, S., Ye, Z.H., Yu, G.C., Yuan, A.F., Yuda, T., Zhang, H.M., Zhang, J.L., Zhang, N.J., Zhang, X.Y., Zhang, Y., YiZhang, Zhaxisangzhu, Zhou, X.X.

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Is the large-scale sidereal anisotropy of the galactic cosmic-ray intensity really instable at TeV energies? von Amenomori, M., Bi, X.J., Chen, D., Chen, W.Y., Cui, S.W., Danzengluobu, Ding, L.K., Ding, X.H., Feng, C.F., Feng, Zhaoyang, Feng, Z.Y., Gou, Q.B., Guo, H.W., Guo, Y.Q., He, H.H., He, Z.T., Hibino, K., Hotta, N., Hu, Haibing, Hu, H.B., Huang, J., Jia, H.Y., Jiang, L., Kajino, F., Kasahara, K., Katayose, Y., Kato, C., Kawata, K., Labaciren, Le, G.M., Li, A.F., Li, W.J., Liu, C., Liu, J.S., Lu, H., Meng, X.R., Mizutani, K., Munakata, K., Nanjo, H., Nishizawa, M., Ohnishi, M., Ohta, I., Ozawa, S., Qian, X.L., Qu, X.B., Saito, T., Saito, T.Y., Sakata, M., Sako, T.K., Shao, J., Shibata, M., Shiomi, A., Shirai, T., Sugimoto, H., Takita, M., Tan, Y.H., Tateyama, N., Torii, S., Tsuchiya, H., Udo, S., Wang, H., Wu, H.R., Xue, L., Yamamoto, Y., Yang, Z., Yasue, S., Yuan, A.F., Yuda, T., Zhai, L.M., Zhang, H.M., Zhang, J.L., Zhang, X.Y., Zhang, Y., Zhang, Yi, Zhang, Ying, Zhaxisangzhu, Zhou, X.X.

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Moon shadow by cosmic rays under the influence of geomagnetic field and search for antiprotons at multi-TeV energies von Amenomori, M., Ayabe, S., Bi, X.J., Chen, D., Cui, S.W., Danzengluobu, Ding, L.K., Ding, X.H., Feng, C.F., Feng, Zhaoyang, Feng, Z.Y., Gao, X.Y., Geng, Q.X., Guo, H.W., He, H.H., He, M., Hibino, K., Hotta, N., Hu, Haibing, Hu, H.B., Huang, J., Huang, Q., Jia, H.Y., Kajino, F., Kasahara, K., Katayose, Y., Kato, C., Kawata, K., Labaciren, Le, G.M., Li, A.F., Li, J.Y., Lou, Y.-Q., Lu, H., Lu, S.L., Meng, X.R., Mizutani, K., Mu, J., Munakata, K., Nagai, A., Nanjo, H., Nishizawa, M., Ohnishi, M., Ohta, I., Onuma, H., Ouchi, T., Ozawa, S., Ren, J.R., Saito, T., Saito, T.Y., Sakata, M., Sako, T.K., Sasaki, T., Shibata, M., Shiomi, A., Shirai, T., Sugimoto, H., Takita, M., Tan, Y.H., Tateyama, N., Torii, S., Tsuchiya, H., Udo, S., Wang, B.S., Wang, H., Wang, X., Wang, Y.G., Wu, H.R., Xue, L., Yamamoto, Y., Yan, C.T., Yang, X.C., Yasue, S., Ye, Z.H., Yu, G.C., Yuan, A.F., Yuda, T., Zhang, H.M., Zhang, J.L., Zhang, N.J., Zhang, X.Y., Zhang, Y., Zhang, Yi, Zhaxisangzhu, Zhou, X.X.

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Sun's shadow by 10 TeV cosmic rays under the influence of solar activity von Amenomori, M, Ayabe, S, Cao, P.Y, Dai, B.Z, Ding, L.K, Feng, Z.Y, Fu, Y, Guo, H.W, He, M, Hibino, K, Hotta, N, Huang, Q, Huo, A.X, Izu, I, Jia, H.Y, Kajino, F, Kasahara, K, Katayose, Y, Labaciren, Li, J.Y, Liu, S.M, Lu, H, Lu, S.L, Luo, G.X, Mei, D.M, Meng, X.R, Mizutani, K, Mu, J, Nanjo, H, Nishizawa, M, Ohnishi, M, Ohta, I, Ouchi, T, Ren, J.R, Saito, To, Sakata, M, Sasaki, T, Shi, C, Shi, Z.Z, Shibata, M, Shiomi, A, Shirai, T, Sugimoto, H, Taira, K, Tan, Y.H, Tateyama, N, Torii, S, Utsugi, T, Wang, C.R, Wang, H, Wang, P.X, Xie, W, Xu, X.W, Yamamoto, Y, Yu, G.C, Yuan, A.F, Yuda, T, Zhang, C.S, Zhang, H.M, Zhang, J.L, Zhang, N.J, Zhang, X.Y, Zhaxisangzhu, Zhaxiciren, Zhou, S.J, Zhou, W.D

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The energy spectrum of all-particle cosmic rays around the knee region observed with the Tibet-III air-shower array von Amenomori, M., Ayabe, S., Bi, X.J., Chen, D., Cui, S.W., Danzengluobu, Ding, L.K., Ding, X.H., Feng, C.F., Feng, Zhaoyang, Feng, Z.Y., Gao, X.Y., Geng, Q.X., Guo, H.W., He, H.H., He, M., Hibino, K., Hotta, N., Hu, Haibing, Hu, H.B., Huang, J., Huang, Q., Jia, H.Y., Kajino, F., Kasahara, K., Katayose, Y., Kato, C., Kawata, K., Labaciren, Le, G.M., Li, A.F., Li, J.Y., Lou, Y.-Q., Lu, H., Lu, S.L., Meng, X.R., Mizutani, K., Mu, J., Munakata, K., Nagai, A., Nanjo, H., Nishizawa, M., Ohnishi, M., Ohta, I., Onuma, H., Ouchi, T., Ozawa, S., Ren, J.R., Saito, T., Saito, T.Y., Sakata, M., Sako, T.K., Sasaki, T., Shibata, M., Shiomi, A., Shirai, T., Sugimoto, H., Takita, M., Tan, Y.H., Tateyama, N., Torii, S., Tsuchiya, H., Udo, S., Wang, B., Wang, H., Wang, X., Wang, Y.G., Wu, H.R., Xue, L., Yamamoto, Y., Yan, C.T., Yang, X.C., Yasue, S., Ye, Z.H., Yu, G.C., Yuan, A.F., Yuda, T., Zhang, H.M., Zhang, J.L., Zhang, N.J., Zhang, X.Y., Zhang, Y., Zhang, Yi, Zhaxisangzhu, Zhou, X.X.

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Flux upper limits of diffuse TeV gamma rays from the Galactic plane using the effective area of the Tibet-II and -III arrays von Amenomori, M., Ayabe, S., Cui, S.W., Danzengluobu, Ding, L.K., Ding, X.H., Feng, C.F., Feng, Z.Y., Gao, X.Y., Geng, Q.X., Guo, H.W., He, H.H., He, M., Hibino, K., Hotta, N., Hu, Haibing, Hu, H.B., Huang, J., Huang, Q., Izumi, M., Jia, H.Y., Kajino, F., Kasahara, K., Katayose, Y., Kato, C., Kawata, K., Labaciren, Le, G.M., Li, J.Y., Lu, H., Lu, S.L., Meng, X.R., Mizutani, K., Mu, J., Munakata, K., Nagai, A., Nanjo, H., Nishizawa, M., Ohnishi, M., Ohta, I., Onuma, H., Ouchi, T., Ozawa, S., Ren, J.R., Saito, T., Sakata, M., Sasaki, T., Shibata, M., Shiomi, A., Shirai, T., Sugimoto, H., Takita, M., Tan, Y.H., Tateyama, N., Torii, S., Tsuchiya, H., Udo, S., Utsugi, T., Wang, B.S., Wang, H., Wang, X., Wang, Y.G., Wu, H.R., Xue, L., Yamamoto, Y., Yan, C.T., Yang, X.C., Yasue, S., Ye, Z.H., Yu, G.C., Yuan, A.F., Yuda, T., Zhang, H.M., Zhang, J.L., Zhang, N.J., Zhang, X.Y., Zhang, Y., Zhaxisangzhu, Zhou, X.X.

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Variation of Sun shadow in the Solar Cycle 23 observed with the Tibet air shower array von Amenomori, M., Ayabe, S., Cui, S.W., Danzengluobu, Ding, L.K., Ding, X.H., Feng, C.F., Feng, Z.Y., Gao, X.Y., Geng, Q.X., Guo, H.W., He, H.H., He, M., Hibino, K., Hotta, N., Hu, Haibing, Hu, H.B., Huang, J., Huang, Q., Izumi, M., Jia, H.Y., Kajino, F., Kasahara, K., Katayose, Y., Kato, C., Kawata, K., Labaciren, Le, G.M., Li, J.Y., Lu, H., Lu, S.L., Meng, X.R., Mizutani, K., Mu, J., Munakata, K., Nagai, A., Nanjo, H., Nishizawa, M., Ohnishi, M., Ohta, I., Onuma, H., Ouchi, T., Ozawa, S., Ren, J.R., Saito, T., Sakata, M., Sasaki, T., Shibata, M., Shiomi, A., Shirai, T., Sugimoto, H., Takita, M., Tan, Y.H., Tateyama, N., Torii, S., Tsuchiya, H., Udo, S., Utsugi, T., Wang, B.S., Wang, H., Wang, X., Wang, Y.G., Wu, H.R., Xue, L., Yamamoto, Y., Yan, C.T., Yang, X.C., Yasue, S., Ye, Z.H., Yu, G.C., Yuan, A.F., Yuda, T., Zhang, H.M., Zhang, J.L., Zhang, N.J., Zhang, X.Y., Zhang, Y., Zhaxisangzhu, Zhou, X.X.

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