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Measurement of the cosmic ray proton spectrum from 40 GeV to 100 TeV with the DAMPE satellite

The precise measurement of the spectrum of protons, the most abundant component of the cosmic radiation, is necessary to understand the source and acceleration of cosmic rays in the Milky Way. This work reports the measurement of the cosmic ray proton fluxes with kinetic energies from 40 GeV to 100...

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Autores principales:	An, Q., Asfandiyarov, R., Azzarello, P., Bernardini, P., Bi, X. J., Cai, M. S., Chang, J., Chen, D. Y., Chen, H. F., Chen, J. L., Chen, W., Cui, M. Y., Cui, T. S., Dai, H. T., D’Amone, A., De Benedittis, A., De Mitri, I., Di Santo, M., Ding, M., Dong, T. K., Dong, Y. F., Dong, Z. X., Donvito, G., Droz, D., Duan, J. L., Duan, K. K., D’Urso, D., Fan, R. R., Fan, Y. Z., Fang, F., Feng, C. Q., Feng, L., Fusco, P., Gallo, V., Gan, F. J., Gao, M., Gargano, F., Gong, K., Gong, Y. Z., Guo, D. Y., Guo, J. H., Guo, X. L., Han, S. X., Hu, Y. M., Huang, G. S., Huang, X. Y., Huang, Y. Y., Ionica, M., Jiang, W., Jin, X., Kong, J., Lei, S. J., Li, S., Li, W. L., Li, X., Li, X. Q., Li, Y., Liang, Y. F., Liang, Y. M., Liao, N. H., Liu, C. M., Liu, H., Liu, J., Liu, S. B., Liu, W. Q., Liu, Y., Loparco, F., Luo, C. N., Ma, M., Ma, P. X., Ma, S. Y., Ma, T., Ma, X. Y., Marsella, G., Mazziotta, M. N., Mo, D., Niu, X. Y., Pan, X., Peng, W. X., Peng, X. Y., Qiao, R., Rao, J. N., Salinas, M. M., Shang, G. Z., Shen, W. H., Shen, Z. Q., Shen, Z. T., Song, J. X., Su, H., Su, M., Sun, Z. Y., Surdo, A., Teng, X. J., Tykhonov, A., Vitillo, S., Wang, C., Wang, H., Wang, H. Y., Wang, J. Z., Wang, L. G., Wang, Q., Wang, S., Wang, X. H., Wang, X. L., Wang, Y. F., Wang, Y. P., Wang, Y. Z., Wang, Z. M., Wei, D. M., Wei, J. J., Wei, Y. F., Wen, S. C., Wu, D., Wu, J., Wu, L. B., Wu, S. S., Wu, X., Xi, K., Xia, Z. Q., Xu, H. T., Xu, Z. H., Xu, Z. L., Xu, Z. Z., Xue, G. F., Yang, H. B., Yang, P., Yang, Y. Q., Yang, Z. L., Yao, H. J., Yu, Y. H., Yuan, Q., Yue, C., Zang, J. J., Zhang, F., Zhang, J. Y., Zhang, J. Z., Zhang, P. F., Zhang, S. X., Zhang, W. Z., Zhang, Y., Zhang, Y. J., Zhang, Y. L., Zhang, Y. P., Zhang, Y. Q., Zhang, Z., Zhang, Z. Y., Zhao, H., Zhao, H. Y., Zhao, X. F., Zhou, C. Y., Zhou, Y., Zhu, X., Zhu, Y., Zimmer, S.
Formato:	Online Artículo Texto
Lenguaje:	English
Publicado:	American Association for the Advancement of Science 2019
Materias:	Research Articles
Acceso en línea:	https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6868675/ https://www.ncbi.nlm.nih.gov/pubmed/31799401 http://dx.doi.org/10.1126/sciadv.aax3793

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author	An, Q. Asfandiyarov, R. Azzarello, P. Bernardini, P. Bi, X. J. Cai, M. S. Chang, J. Chen, D. Y. Chen, H. F. Chen, J. L. Chen, W. Cui, M. Y. Cui, T. S. Dai, H. T. D’Amone, A. De Benedittis, A. De Mitri, I. Di Santo, M. Ding, M. Dong, T. K. Dong, Y. F. Dong, Z. X. Donvito, G. Droz, D. Duan, J. L. Duan, K. K. D’Urso, D. Fan, R. R. Fan, Y. Z. Fang, F. Feng, C. Q. Feng, L. Fusco, P. Gallo, V. Gan, F. J. Gao, M. Gargano, F. Gong, K. Gong, Y. Z. Guo, D. Y. Guo, J. H. Guo, X. L. Han, S. X. Hu, Y. M. Huang, G. S. Huang, X. Y. Huang, Y. Y. Ionica, M. Jiang, W. Jin, X. Kong, J. Lei, S. J. Li, S. Li, W. L. Li, X. Li, X. Q. Li, Y. Liang, Y. F. Liang, Y. M. Liao, N. H. Liu, C. M. Liu, H. Liu, J. Liu, S. B. Liu, W. Q. Liu, Y. Loparco, F. Luo, C. N. Ma, M. Ma, P. X. Ma, S. Y. Ma, T. Ma, X. Y. Marsella, G. Mazziotta, M. N. Mo, D. Niu, X. Y. Pan, X. Peng, W. X. Peng, X. Y. Qiao, R. Rao, J. N. Salinas, M. M. Shang, G. Z. Shen, W. H. Shen, Z. Q. Shen, Z. T. Song, J. X. Su, H. Su, M. Sun, Z. Y. Surdo, A. Teng, X. J. Tykhonov, A. Vitillo, S. Wang, C. Wang, H. Wang, H. Y. Wang, J. Z. Wang, L. G. Wang, Q. Wang, S. Wang, X. H. Wang, X. L. Wang, Y. F. Wang, Y. P. Wang, Y. Z. Wang, Z. M. Wei, D. M. Wei, J. J. Wei, Y. F. Wen, S. C. Wu, D. Wu, J. Wu, L. B. Wu, S. S. Wu, X. Xi, K. Xia, Z. Q. Xu, H. T. Xu, Z. H. Xu, Z. L. Xu, Z. Z. Xue, G. F. Yang, H. B. Yang, P. Yang, Y. Q. Yang, Z. L. Yao, H. J. Yu, Y. H. Yuan, Q. Yue, C. Zang, J. J. Zhang, F. Zhang, J. Y. Zhang, J. Z. Zhang, P. F. Zhang, S. X. Zhang, W. Z. Zhang, Y. Zhang, Y. J. Zhang, Y. L. Zhang, Y. P. Zhang, Y. Q. Zhang, Z. Zhang, Z. Y. Zhao, H. Zhao, H. Y. Zhao, X. F. Zhou, C. Y. Zhou, Y. Zhu, X. Zhu, Y. Zimmer, S.
author_facet	An, Q. Asfandiyarov, R. Azzarello, P. Bernardini, P. Bi, X. J. Cai, M. S. Chang, J. Chen, D. Y. Chen, H. F. Chen, J. L. Chen, W. Cui, M. Y. Cui, T. S. Dai, H. T. D’Amone, A. De Benedittis, A. De Mitri, I. Di Santo, M. Ding, M. Dong, T. K. Dong, Y. F. Dong, Z. X. Donvito, G. Droz, D. Duan, J. L. Duan, K. K. D’Urso, D. Fan, R. R. Fan, Y. Z. Fang, F. Feng, C. Q. Feng, L. Fusco, P. Gallo, V. Gan, F. J. Gao, M. Gargano, F. Gong, K. Gong, Y. Z. Guo, D. Y. Guo, J. H. Guo, X. L. Han, S. X. Hu, Y. M. Huang, G. S. Huang, X. Y. Huang, Y. Y. Ionica, M. Jiang, W. Jin, X. Kong, J. Lei, S. J. Li, S. Li, W. L. Li, X. Li, X. Q. Li, Y. Liang, Y. F. Liang, Y. M. Liao, N. H. Liu, C. M. Liu, H. Liu, J. Liu, S. B. Liu, W. Q. Liu, Y. Loparco, F. Luo, C. N. Ma, M. Ma, P. X. Ma, S. Y. Ma, T. Ma, X. Y. Marsella, G. Mazziotta, M. N. Mo, D. Niu, X. Y. Pan, X. Peng, W. X. Peng, X. Y. Qiao, R. Rao, J. N. Salinas, M. M. Shang, G. Z. Shen, W. H. Shen, Z. Q. Shen, Z. T. Song, J. X. Su, H. Su, M. Sun, Z. Y. Surdo, A. Teng, X. J. Tykhonov, A. Vitillo, S. Wang, C. Wang, H. Wang, H. Y. Wang, J. Z. Wang, L. G. Wang, Q. Wang, S. Wang, X. H. Wang, X. L. Wang, Y. F. Wang, Y. P. Wang, Y. Z. Wang, Z. M. Wei, D. M. Wei, J. J. Wei, Y. F. Wen, S. C. Wu, D. Wu, J. Wu, L. B. Wu, S. S. Wu, X. Xi, K. Xia, Z. Q. Xu, H. T. Xu, Z. H. Xu, Z. L. Xu, Z. Z. Xue, G. F. Yang, H. B. Yang, P. Yang, Y. Q. Yang, Z. L. Yao, H. J. Yu, Y. H. Yuan, Q. Yue, C. Zang, J. J. Zhang, F. Zhang, J. Y. Zhang, J. Z. Zhang, P. F. Zhang, S. X. Zhang, W. Z. Zhang, Y. Zhang, Y. J. Zhang, Y. L. Zhang, Y. P. Zhang, Y. Q. Zhang, Z. Zhang, Z. Y. Zhao, H. Zhao, H. Y. Zhao, X. F. Zhou, C. Y. Zhou, Y. Zhu, X. Zhu, Y. Zimmer, S.
collection	PubMed
description	The precise measurement of the spectrum of protons, the most abundant component of the cosmic radiation, is necessary to understand the source and acceleration of cosmic rays in the Milky Way. This work reports the measurement of the cosmic ray proton fluxes with kinetic energies from 40 GeV to 100 TeV, with 2 (1)/(2) years of data recorded by the DArk Matter Particle Explorer (DAMPE). This is the first time that an experiment directly measures the cosmic ray protons up to ~100 TeV with high statistics. The measured spectrum confirms the spectral hardening at ~300 GeV found by previous experiments and reveals a softening at ~13.6 TeV, with the spectral index changing from ~2.60 to ~2.85. Our result suggests the existence of a new spectral feature of cosmic rays at energies lower than the so-called knee and sheds new light on the origin of Galactic cosmic rays.
format	Online Article Text
id	pubmed-6868675
institution	National Center for Biotechnology Information
language	English
publishDate	2019
publisher	American Association for the Advancement of Science
record_format	MEDLINE/PubMed
spelling	pubmed-68686752019-12-03 Measurement of the cosmic ray proton spectrum from 40 GeV to 100 TeV with the DAMPE satellite An, Q. Asfandiyarov, R. Azzarello, P. Bernardini, P. Bi, X. J. Cai, M. S. Chang, J. Chen, D. Y. Chen, H. F. Chen, J. L. Chen, W. Cui, M. Y. Cui, T. S. Dai, H. T. D’Amone, A. De Benedittis, A. De Mitri, I. Di Santo, M. Ding, M. Dong, T. K. Dong, Y. F. Dong, Z. X. Donvito, G. Droz, D. Duan, J. L. Duan, K. K. D’Urso, D. Fan, R. R. Fan, Y. Z. Fang, F. Feng, C. Q. Feng, L. Fusco, P. Gallo, V. Gan, F. J. Gao, M. Gargano, F. Gong, K. Gong, Y. Z. Guo, D. Y. Guo, J. H. Guo, X. L. Han, S. X. Hu, Y. M. Huang, G. S. Huang, X. Y. Huang, Y. Y. Ionica, M. Jiang, W. Jin, X. Kong, J. Lei, S. J. Li, S. Li, W. L. Li, X. Li, X. Q. Li, Y. Liang, Y. F. Liang, Y. M. Liao, N. H. Liu, C. M. Liu, H. Liu, J. Liu, S. B. Liu, W. Q. Liu, Y. Loparco, F. Luo, C. N. Ma, M. Ma, P. X. Ma, S. Y. Ma, T. Ma, X. Y. Marsella, G. Mazziotta, M. N. Mo, D. Niu, X. Y. Pan, X. Peng, W. X. Peng, X. Y. Qiao, R. Rao, J. N. Salinas, M. M. Shang, G. Z. Shen, W. H. Shen, Z. Q. Shen, Z. T. Song, J. X. Su, H. Su, M. Sun, Z. Y. Surdo, A. Teng, X. J. Tykhonov, A. Vitillo, S. Wang, C. Wang, H. Wang, H. Y. Wang, J. Z. Wang, L. G. Wang, Q. Wang, S. Wang, X. H. Wang, X. L. Wang, Y. F. Wang, Y. P. Wang, Y. Z. Wang, Z. M. Wei, D. M. Wei, J. J. Wei, Y. F. Wen, S. C. Wu, D. Wu, J. Wu, L. B. Wu, S. S. Wu, X. Xi, K. Xia, Z. Q. Xu, H. T. Xu, Z. H. Xu, Z. L. Xu, Z. Z. Xue, G. F. Yang, H. B. Yang, P. Yang, Y. Q. Yang, Z. L. Yao, H. J. Yu, Y. H. Yuan, Q. Yue, C. Zang, J. J. Zhang, F. Zhang, J. Y. Zhang, J. Z. Zhang, P. F. Zhang, S. X. Zhang, W. Z. Zhang, Y. Zhang, Y. J. Zhang, Y. L. Zhang, Y. P. Zhang, Y. Q. Zhang, Z. Zhang, Z. Y. Zhao, H. Zhao, H. Y. Zhao, X. F. Zhou, C. Y. Zhou, Y. Zhu, X. Zhu, Y. Zimmer, S. Sci Adv Research Articles The precise measurement of the spectrum of protons, the most abundant component of the cosmic radiation, is necessary to understand the source and acceleration of cosmic rays in the Milky Way. This work reports the measurement of the cosmic ray proton fluxes with kinetic energies from 40 GeV to 100 TeV, with 2 (1)/(2) years of data recorded by the DArk Matter Particle Explorer (DAMPE). This is the first time that an experiment directly measures the cosmic ray protons up to ~100 TeV with high statistics. The measured spectrum confirms the spectral hardening at ~300 GeV found by previous experiments and reveals a softening at ~13.6 TeV, with the spectral index changing from ~2.60 to ~2.85. Our result suggests the existence of a new spectral feature of cosmic rays at energies lower than the so-called knee and sheds new light on the origin of Galactic cosmic rays. American Association for the Advancement of Science 2019-09-27 /pmc/articles/PMC6868675/ /pubmed/31799401 http://dx.doi.org/10.1126/sciadv.aax3793 Text en Copyright © 2019 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. No claim to original U.S. Government Works. Distributed under a Creative Commons Attribution NonCommercial License 4.0 (CC BY-NC). http://creativecommons.org/licenses/by-nc/4.0/ This is an open-access article distributed under the terms of the Creative Commons Attribution-NonCommercial license (http://creativecommons.org/licenses/by-nc/4.0/) , which permits use, distribution, and reproduction in any medium, so long as the resultant use is not for commercial advantage and provided the original work is properly cited.
spellingShingle	Research Articles An, Q. Asfandiyarov, R. Azzarello, P. Bernardini, P. Bi, X. J. Cai, M. S. Chang, J. Chen, D. Y. Chen, H. F. Chen, J. L. Chen, W. Cui, M. Y. Cui, T. S. Dai, H. T. D’Amone, A. De Benedittis, A. De Mitri, I. Di Santo, M. Ding, M. Dong, T. K. Dong, Y. F. Dong, Z. X. Donvito, G. Droz, D. Duan, J. L. Duan, K. K. D’Urso, D. Fan, R. R. Fan, Y. Z. Fang, F. Feng, C. Q. Feng, L. Fusco, P. Gallo, V. Gan, F. J. Gao, M. Gargano, F. Gong, K. Gong, Y. Z. Guo, D. Y. Guo, J. H. Guo, X. L. Han, S. X. Hu, Y. M. Huang, G. S. Huang, X. Y. Huang, Y. Y. Ionica, M. Jiang, W. Jin, X. Kong, J. Lei, S. J. Li, S. Li, W. L. Li, X. Li, X. Q. Li, Y. Liang, Y. F. Liang, Y. M. Liao, N. H. Liu, C. M. Liu, H. Liu, J. Liu, S. B. Liu, W. Q. Liu, Y. Loparco, F. Luo, C. N. Ma, M. Ma, P. X. Ma, S. Y. Ma, T. Ma, X. Y. Marsella, G. Mazziotta, M. N. Mo, D. Niu, X. Y. Pan, X. Peng, W. X. Peng, X. Y. Qiao, R. Rao, J. N. Salinas, M. M. Shang, G. Z. Shen, W. H. Shen, Z. Q. Shen, Z. T. Song, J. X. Su, H. Su, M. Sun, Z. Y. Surdo, A. Teng, X. J. Tykhonov, A. Vitillo, S. Wang, C. Wang, H. Wang, H. Y. Wang, J. Z. Wang, L. G. Wang, Q. Wang, S. Wang, X. H. Wang, X. L. Wang, Y. F. Wang, Y. P. Wang, Y. Z. Wang, Z. M. Wei, D. M. Wei, J. J. Wei, Y. F. Wen, S. C. Wu, D. Wu, J. Wu, L. B. Wu, S. S. Wu, X. Xi, K. Xia, Z. Q. Xu, H. T. Xu, Z. H. Xu, Z. L. Xu, Z. Z. Xue, G. F. Yang, H. B. Yang, P. Yang, Y. Q. Yang, Z. L. Yao, H. J. Yu, Y. H. Yuan, Q. Yue, C. Zang, J. J. Zhang, F. Zhang, J. Y. Zhang, J. Z. Zhang, P. F. Zhang, S. X. Zhang, W. Z. Zhang, Y. Zhang, Y. J. Zhang, Y. L. Zhang, Y. P. Zhang, Y. Q. Zhang, Z. Zhang, Z. Y. Zhao, H. Zhao, H. Y. Zhao, X. F. Zhou, C. Y. Zhou, Y. Zhu, X. Zhu, Y. Zimmer, S. Measurement of the cosmic ray proton spectrum from 40 GeV to 100 TeV with the DAMPE satellite
title	Measurement of the cosmic ray proton spectrum from 40 GeV to 100 TeV with the DAMPE satellite
title_full	Measurement of the cosmic ray proton spectrum from 40 GeV to 100 TeV with the DAMPE satellite
title_fullStr	Measurement of the cosmic ray proton spectrum from 40 GeV to 100 TeV with the DAMPE satellite
title_full_unstemmed	Measurement of the cosmic ray proton spectrum from 40 GeV to 100 TeV with the DAMPE satellite
title_short	Measurement of the cosmic ray proton spectrum from 40 GeV to 100 TeV with the DAMPE satellite
title_sort	measurement of the cosmic ray proton spectrum from 40 gev to 100 tev with the dampe satellite
topic	Research Articles
url	https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6868675/ https://www.ncbi.nlm.nih.gov/pubmed/31799401 http://dx.doi.org/10.1126/sciadv.aax3793
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measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT suh measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT sum measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT sunzy measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT surdoa measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT tengxj measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT tykhonova measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT vitillos measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT wangc measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT wangh measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT wanghy measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT wangjz measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT wanglg measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT wangq measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT wangs measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT wangxh measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT wangxl measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT wangyf measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT wangyp measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT wangyz measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT wangzm measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT weidm measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT weijj measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT weiyf measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT wensc measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT wud measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT wuj measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT wulb measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT wuss measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT wux measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT xik measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT xiazq measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT xuht measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT xuzh measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT xuzl measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT xuzz measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT xuegf measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT yanghb measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT yangp measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT yangyq measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT yangzl measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT yaohj measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT yuyh measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT yuanq measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT yuec measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT zangjj measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT zhangf measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT zhangjy measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT zhangjz measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT zhangpf measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT zhangsx measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT zhangwz measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT zhangy measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT zhangyj measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT zhangyl measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT zhangyp measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT zhangyq measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT zhangz measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT zhangzy measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT zhaoh measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT zhaohy measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT zhaoxf measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT zhoucy measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT zhouy measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT zhux measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT zhuy measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite AT zimmers measurementofthecosmicrayprotonspectrumfrom40gevto100tevwiththedampesatellite

Measurement of the cosmic ray proton spectrum from 40 GeV to 100 TeV with the DAMPE satellite

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