المؤلفون: Vainio, R., Zuccon, P., Zichichi, A., Zhukov, V., Zhuang, H.L., Zheng, Z.M., Zheng, C., Zhao, F., Zhang, Z., Zhang, J.H., Zhang, J., Zhang, F.Z., Zhang, F., Zhang, C., Yu, Z.Q., Yu, Y.M., You, Y.H., Yi, H., Yelland, A., Yang, Y., Yang, H.T., Yan, Q., Xu, W., Xiong, X.Z., Xiong, R.Q., Xiao, J.N., Wu, Y., Wu, H., Weng, Z.L., Wei, J., Wang, Z.M., Wang, Yu, Wang, X., Wang, S., Wang, Q.L., Wang, N.H., Wang, L.Q., Wang, L., Wang, C.X., Vialle, J.P., Velasco, M., Vecchi, M., Torsti, J., Urban, T., Usoskin, I., Vagelli, V., Vázquez Acosta, M., Valtonen, E., Valente, E., Valencia-Otero, M., Demirköz, MELAHAT BİLGE, Aguilar, M., Ambrosi, G., Anderson, H., Arruda, L., Attig, N., Bagwell, C., Barao, F., Barbanera, M., Barrin, L., Bartoloni, A., Battiston, R., Belyaev, N., Berdugo, J., Bertucci, B., Bindi, V., Bollweg, K., Bolster, J., Borchiellini, M., Borgia, B., Boschini, M.J., Bourquin, M., Burger, J., Burger, W.J., Cai, X.D., Capell, M., Casaus, J., Castellini, G., Cervelli, F., Chang, Y.H., Chen, G.M., Chen, G.R., Chen, H., Chen, H.S., Chen, Y., Cheng, L., Chou, H.Y., Chouridou, S., Choutko, V., Chung, C.H., Clark, C., Coignet, G., Consolandi, C., Contin, A., Corti, C., Cui, Z., Dadzie, K., D'Angelo, F., Dass, A., Delgado, C., Della Torre, S., Derome, L., Di Falco, S., Di Felice, V., Díaz, C., Dimiccoli, F., von Doetinchem, P., Dong, F., Donnini, F., Duranti, M., Egorov, A., Eline, A., Faldi, F., Feng, J., Fiandrini, E., Fisher, P., Formato, V., Gámez, C., García-López, R.J., Gargiulo, C., Gast, H., Gervasi, M., Giovacchini, F., Gómez-Coral, D.M., Gong, J., Goy, C., Grandi, D., Graziani, M., Guracho, A.N., Haino, S., Han, K.C., Hashmani, R.K., He, Z.H., Heber, B., Hsieh, T.H., Hu, J.Y., Huang, B.W., Ionica, M., Incagli, M., Jia, Yi, Jinchi, H., Karagöz, G., Khan, S., Khiali, B., Kirn, Th, Klipfel, A.P., Kounina, O., Kounine, A., Koutsenko, V., Krasnopevtsev, D., Kuhlman, A., Kulemzin, A., La Vacca, G., Laudi, E., Laurenti, G., LaVecchia, G., Lazzizzera, I., Lee, H.T., Lee, S.C., Li, H.L., Li, J.Q., Li, M., Li, Q., Li, Q.Y., Li, S., Li, S.L., Li, J.H., Li, Z.H., Liang, J., Liang, M.J., Lin, C.H., Lippert, T., Liu, J.H., Lu, S.Q., Lu, Y.S., Luebelsmeyer, K., Luo, J.Z., Luo, S.D., Luo, Xi, Mañá, C., Marín, J., Marquardt, J., Martin, T., Martínez, G., Masi, N., Maurin, D., Medvedeva, T., Menchaca-Rocha, A., Meng, Q., Molero, M., Mott, P., Mussolin, L., Jozani, Y Najafi, Negrete, J., Nicolaidis, R., Nikonov, N., Nozzoli, F., Ocampo-Peleteiro, J., Oliva, A., Orcinha, M., Ottupara, M.A., Palermo, M., Palmonari, F., Paniccia, M., Pashnin, A., Pauluzzi, M., Pensotti, S., Plyaskin, V., Poluianov, S., Qin, X., Qu, Z.Y., Quadrani, L., Rancoita, P.G., Rapin, D., Conde, A Reina, Robyn, E., Rodríguez-García, I., Romaneehsen, L., Rossi, F., Rozhkov, A., Rozza, D., Sagdeev, R., Savin, E., Schael, S., von Dratzig, A Schultz, Schwering, G., Seo, E.S., Shan, B.S., Siedenburg, T., Silvestre, G., Song, J.W., Song, X.J., Sonnabend, R., Strigari, L., Su, T., Sun, Q., Sun, Z.T., Tacconi, M., Tang, X.W., Tang, Z.C., Tian, J., Tian, Y., Ting, Samuel C C, Ting, S.M., Tomassetti, N.

الوصف: We present the precision measurements of 11 years of daily cosmic positron fluxes in the rigidity range from 1.00 to 41.9 GV based on 3.4 x 106 positrons collected with the Alpha Magnetic Spectrometer (AMS) aboard the International Space Station. The positron fluxes show distinctly different time variations from the electron fluxes at short and long timescales. A hysteresis between the electron fluxes and the positron fluxes is observed with a significance greater than 5 sigma at rigidities below 8.5 GV. On the contrary, the positron fluxes and the proton fluxes show similar time variation. Remarkably, we found that positron fluxes are modulated more than proton fluxes with a significance greater than 5 sigma for rigidities below 7 GV. These continuous daily positron fluxes, together with AMS daily electron, proton, and helium fluxes over an 11-year solar cycle, provide unique input to the understanding of both the charge-sign and mass dependencies of cosmic rays in the heliosphere.

العلاقة: b7a8c75b-7af2-4c52-8094-b21eb88dfa01; https://avesis.metu.edu.tr/publication/details/b7a8c75b-7af2-4c52-8094-b21eb88dfa01/oaiTest

الإتاحة: https://doi.org/10.1103/physrevlett.131.151002Test
https://avesis.metu.edu.tr/publication/details/b7a8c75b-7af2-4c52-8094-b21eb88dfa01/oaiTest

المؤلفون: Ambrosi, G., Bertucci, B., Bollweg, K., Burger, J., Cai, X., Capell, M., Chung, C.H., Chuang, Y.R., Clark, C., Ding, T., FanChiang, Y.J., Gargiulo, C., Gaggiotti, M., Guo, L., He, Z.H., Heil, M., Heilig, J., Karpinski, W., Koutsenko, V., Kulemzin, A., Lübelsmeyer, K., Martin, T., Mo, D.C., Morelli, G., Miao, J.Y., Mott, P., Mussolin, L., Schael, S., von Dratzig, A. Schutlz, Schwering, G., Scolieri, G., Siedenburg, T., Solano, C., Urban, T., Verlaat, B., Wang, S.H., Wlochal, M., Yan, J.J., Yang, Y., Yu, Y.M., Zeng, R.C., Zhang, Z.

المصدر: Applied Thermal Engineering ; volume 230, page 120738 ; ISSN 1359-4311

مصطلحات موضوعية: Industrial and Manufacturing Engineering, Energy Engineering and Power Technology, Fluid Flow and Transfer Processes, Mechanical Engineering

الإتاحة: https://doi.org/10.1016/j.applthermaleng.2023.120738Test
https://api.elsevier.com/content/article/PII:S1359431123007676?httpAccept=text/xmlTest
https://api.elsevier.com/content/article/PII:S1359431123007676?httpAccept=text/plainTest

المؤلفون: Aguilar, M, Alpat, B, Ambrosi, G, Anderson, H, Arruda, L, Attig, N, Bagwell, C, Barao, F, Barbanera, M, Barrin, L, Bartoloni, A, Battiston, R, Bayyari, A, Belyaev, N, Bertucci, B, Bindi, V, Bollweg, K, Bolster, J, Borchiellini, M, Borgia, B, Boschini, M.J, Bourquin, M, Brugnoni, C, Burger, J, Burger, W.J, Cai, X.D, Capell, M, Casaus, J, Castellini, G, Cervelli, F, Chang, Y.H, Chen, G.M, Chen, G.R, Chen, H, Chen, H.S, Chen, Y, Cheng, L, Chou, H.Y, Chouridou, S, Choutko, V, Chung, C.H, Clark, C, Coignet, G, Consolandi, C, Contin, A, Corti, C, Cui, Z, Dadzie, K, d'Angelo, F, Dass, A, Delgado, C, Della Torre, S, Demirköz, M.B, Derome, L, Di Falco, S, Di Felice, V, Díaz, C, Dimiccoli, F, von Doetinchem, P, Dong, F, Donnini, F, Duranti, M, Egorov, A, Eline, A, Faldi, F, Fehr, D, Feng, J, Fiandrini, E, Fisher, P, Formato, V, Gámez, C, García-López, R.J, Gargiulo, C, Gast, H, Gervasi, M, Giovacchini, F, Gómez-Coral, D.M, Gong, J, Grandi, D, Graziani, M, Guracho, A.N, Haino, S, Han, K.C, Hashmani, R.K, He, Z.H, Heber, B, Hsieh, T.H, Hu, J.Y, Huang, B.W, Ionica, M, Incagli, M, Jia, Yi, Jinchi, H, Karagöz, G, Khan, S, Khiali, B, Kirn, Th, Klipfel, A.P, Kounina, O, Kounine, A, Koutsenko, V, Krasnopevtsev, D, Kuhlman, A, Kulemzin, A, La Vacca, G, Laudi, E, Laurenti, G, Lavecchia, G, Lazzizzera, I, Lee, H.T, Lee, S.C, Li, H.L, Li, J.Q, Li, M, Li, Q, Li, Q.Y, Li, S, Li, S.L, Li, J.H, Li, Z.H, Liang, M.J, Liao, P, Lin, C.H, Lippert, T, Liu, J.H, Liu, P.C, Lu, S.Q, Lu, Y.S, Luebelsmeyer, K, Luo, J.Z, Luo, Q, Luo, S.D, Luo, Xi, Mañá, C, Marín, J, Marquardt, J, Martínez, G, Masi, N, Maurin, D, Medvedeva, T, Menchaca-Rocha, A, Meng, Q, Mikhailov, V.V, Molero, M, Mott, P, Mussolin, L, Jozani, Y. Najafi, Nicolaidis, R, Nikonov, N, Nozzoli, F, Ocampo-Peleteiro, J, Oliva, A, Orcinha, M, Palmonari, F, Paniccia, M, Pashnin, A, Pauluzzi, M, Pensotti, S, Pietzcker, P, Plyaskin, V, Poluianov, S, Pridöhl, D, Qu, Z.Y, Quadrani, L, Rancoita, P.G, Rapin, D, Conde, A. Reina, Robyn, E, Rodríguez-García, I, Romaneehsen, L, Rossi, F, Rozhkov, A, Rozza, D, Sagdeev, R, Savin, E, Schael, S, Schultz von Dratzig, A, Schwering, G, Seo, E.S, Shan, B.S, Shukla, A, Siedenburg, T, Silvestre, G, Song, J.W, Song, X.J, Sonnabend, R, Strigari, L, Su, T, Sun, Q, Sun, Z.T, Tabarroni, L, Tacconi, M, Tang, Z.C, Tian, J, Tian, Y, Ting, Samuel C.C, Ting, S.M, Tomassetti, N, Torsti, J, Urban, T, Usoskin, I, Vagelli, V, Vainio, R, Valencia-Otero, M, Valente, E, Valtonen, E, Vázquez Acosta, M, Vecchi, M, Velasco, M, Wang, C.X, Wang, L, Wang, L.Q, Wang, N.H, Wang, Q.L, Wang, S, Wang, X, Wang, Z.M, Wei, J, Weng, Z.L, Wu, H, Wu, Y, Wu, Z.B, Xiao, J.N, Xiong, R.Q, Xiong, X.Z, Xu, W, Yan, Q, Yang, H.T, Yang, Y, Yelland, A, Yi, H, You, Y.H, Yu, Y.M, Yu, Z.Q, Zhang, C, Zhang, F.Z, Zhang, J, Zhang, J.H, Zhang, Z, Zhao, P.W, Zheng, C, Zheng, Z.M, Zhuang, H.L, Zhukov, V, Zichichi, A, Zuccon, P

المساهمون: Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), AMS

المصدر: Phys.Rev.Lett. ; https://hal.science/hal-04626709Test ; Phys.Rev.Lett., 2024, 132 (26), pp.261001. ⟨10.1103/PhysRevLett.132.261001⟩

مصطلحات موضوعية: flux, ratio, cosmic radiation, propagation, deuteron, magnetic spectrometer, AMS, nucleus, satellite, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]

الوصف: International audience ; Precision measurements by the Alpha Magnetic Spectrometer (AMS) on the International Space Station of the deuteron ( D ) flux are presented. The measurements are based on 21 × 10 6 D nuclei in the rigidity range from 1.9 to 21 GV collected from May 2011 to April 2021. We observe that over the entire rigidity range the D flux exhibits nearly identical time variations with the p , He 3 , and He 4 fluxes. Above 4.5 GV, the D / He 4 flux ratio is time independent and its rigidity dependence is well described by a single power law ∝ R Δ with Δ D / He 4 = - 0.108 ± 0.005 . This is in contrast with the He 3 / He 4 flux ratio for which we find Δ He 3 / He 4 = - 0.289 ± 0.003 . Above ∼ 13 GV we find a nearly identical rigidity dependence of the D and p fluxes with a D / p flux ratio of 0.027 ± 0.001 . These unexpected observations indicate that cosmic deuterons have a sizable primarylike component. With a method independent of cosmic ray propagation, we obtain the primary component of the D flux equal to 9.4 ± 0.5 % of the He 4 flux and the secondary component of the D flux equal to 58 ± 5 % of the He 3 flux.

العلاقة: hal-04626709; https://hal.science/hal-04626709Test; INSPIRE: 2802516

الإتاحة: https://doi.org/10.1103/PhysRevLett.132.261001Test
https://hal.science/hal-04626709Test

المؤلفون: Ye, X.B., He, Z.H.

المساهمون: Fujian Provincial Natural Science Foundation, National Natural Science Foundation of China

المصدر: Materials Today Communications ; volume 39, page 108862 ; ISSN 2352-4928

مصطلحات موضوعية: Materials Chemistry, Mechanics of Materials, General Materials Science

الإتاحة: https://doi.org/10.1016/j.mtcomm.2024.108862Test
https://api.elsevier.com/content/article/PII:S2352492824008432?httpAccept=text/xmlTest
https://api.elsevier.com/content/article/PII:S2352492824008432?httpAccept=text/plainTest

المؤلفون: Dass, A., Dadzie, K., Cui, Z., Corti, C., Contin, A., Consolandi, C., Coignet, G., Clark, C., Chung, C.H., Choutko, V., Chouridou, S., Chou, H.Y., Cheng, L., Chen, Y., Chen, H.S., Başeǧmez-Du Pree, S., Battiston, R., Behlmann, M., Berdugo, J., Bertucci, B., Bindi, V., Bollweg, K., Borgia, B., Boschini, M.J., Bourquin, M., Bueno, E.F., Burger, J., Burger, W.J., Burmeister, S., Medvedeva, T., Maurin, D., Masi, N., Martínez, G., Martin, T., Marquardt, J., Marín, J., Valente, E., Vázquez Acosta, M., Vecchi, M., Velasco, M., Vialle, J.P., Wang, C.X., Wang, L., Wang, L.Q., Wang, N.H., Wang, Q.L., Wang, S., Wang, X., Wang, Yu, Wang, Z.M., Wei, J., Weng, Z.L., Wu, H., Xiong, R.Q., Xu, W., Yan, Q., Yang, Y., Yashin, I.I., Yi, H., Yu, Y.M., Yu, Z.Q., Zannoni, M., Zhang, C., Zhang, F., Zhang, F.Z., Zhang, J.H., Zhang, Z., Zhao, F., Zheng, C., Zheng, Z.M., Zhuang, H.L., Zhukov, V., Zichichi, A., Zuccon, P., Demirköz, MELAHAT BİLGE, Cai, X.D., Capell, M., Casaus, J., Castellini, G., Cervelli, F., Chang, Y.H., Chen, G.M., Chen, G.R., Kounina, O., Konyushikhin, M., Kirn, Th., Kim, G.N., Khiali, B., Karagöz, G., Jinchi, H., Jia, Yi, Jang, W.Y., Incagli, M., Hu, J.Y., Hsieh, T.H., Heber, B., He, Z.H., Hashmani, R.K., Han, K.C., Haino, S., Graziani, M., Grandi, D., Grabski, V., Goy, C., Gong, J., Gómez-Coral, D.M., Giovacchini, F., Gervasi, M., Gast, H., Gargiulo, C., García-López, R.J., Gámez, C., Freeman, C., Formato, V., Fisher, P., Fiandrini, E., Feng, J., Eline, A., Egorov, A., Duranti, M., Donnini, F., Dong, F., Von Doetinchem, P., Dimiccoli, F., Díaz, C., Di Felice, V., Di Falco, S., Derome, L., Della Torre, S., Delgado, C., Siedenburg, T., Song, J.W., Song, X.J., Sonnabend, R., Strigari, L., Su, T., Sun, Q., Sun, Z.T., Tacconi, M., Tang, X.W., Tang, Z.C., Tian, J., Ting, Samuel C. C., Ting, S.M., Tomassetti, N., Torsti, J., Urban, T., Usoskin, I., Vagelli, V., Vainio, R., Valencia-Otero, M., Valtonen, E., Mañá, C., Machate, F., Luo, Xi, Luo, J.Z., Luebelsmeyer, K., Lu, Y.S., Lu, S.Q., Liu, J.H., Lippert, T., Lin, C.H., Light, C., Liang, M.J., Liang, J., Li, Z.H., Li, J.H., Li, S.L., Li, S., Li, Q.Y., Li, Q., Li, M., Li, J.Q., Li, H.L., Lee, S.C., Lee, H.T., Lazzizzera, I., Laurenti, G., Laudi, E., La Vacca, G., Kulemzin, A., Kuhlman, A., Krasnopevtsev, D., Aguilar, M., Cavasonza, L. Ali, Ambrosi, G., Arruda, L., Attig, N., Barao, F., Barrin, L., Bartoloni, A., Koutsenko, V., Kounine, A., Menchaca-Rocha, A., Meng, Q., Mikhailov, V.V., Molero, M., Mott, P., Mussolin, L., Negrete, J., Nikonov, N., Nozzoli, F., Ocampo-Peleteiro, J., Oliva, A., Orcinha, M., Palermo, M., Palmonari, F., Paniccia, M., Pashnin, A., Pauluzzi, M., Pensotti, S., Plyaskin, V., Pohl, M., Poluianov, S., Qin, X., Qu, Z.Y., Quadrani, L., Rancoita, P.G., Rapin, D., Conde, A. Reina, Robyn, E., Rosier-Lees, S., Rozhkov, A., Rozza, D., Sagdeev, R., Schael, S., Von Dratzig, A. Schultz, Schwering, G., Seo, E.S., Shan, B.S.

الوصف: © 2022 authors. Published by the American Physical Society.We present the precision measurement of 2824 daily helium fluxes in cosmic rays from May 20, 2011 to October 29, 2019 in the rigidity interval from 1.71 to 100 GV based on 7.6×108 helium nuclei collected with the Alpha Magnetic Spectrometer (AMS) aboard the International Space Station. The helium flux and the helium to proton flux ratio exhibit variations on multiple timescales. In nearly all the time intervals from 2014 to 2018, we observed recurrent helium flux variations with a period of 27 days. Shorter periods of 9 days and 13.5 days are observed in 2016. The strength of all three periodicities changes with time and rigidity. In the entire time period, we found that below ∼7 GV the helium flux exhibits larger time variations than the proton flux, and above ∼7 GV the helium to proton flux ratio is time independent. Remarkably, below 2.4 GV a hysteresis between the helium to proton flux ratio and the helium flux was observed at greater than the 7σ level. This shows that at low rigidity the modulation of the helium to proton flux ratio is different before and after the solar maximum in 2014.

العلاقة: 236cdedc-7ba7-4ceb-ab44-f2962cefe6c0; https://avesis.metu.edu.tr/publication/details/236cdedc-7ba7-4ceb-ab44-f2962cefe6c0/oaiTest

الإتاحة: https://doi.org/10.1103/physrevlett.128.231102Test
https://avesis.metu.edu.tr/publication/details/236cdedc-7ba7-4ceb-ab44-f2962cefe6c0/oaiTest

المؤلفون: Sun, Q., Sun, Z.T., Tacconi, M., Tang, X.W., Tang, Z.C., Tian, J., Ting, Samuel C. C., Ting, S.M., Tomassetti, N., Torsti, J., Urban, T., Usoskin, I., Vagelli, V., Vainio, R., Valencia-Otero, M., Valente, E., Valtonen, E., Vázquez Acosta, M., Vecchi, M., Velasco, M., Vialle, J.P., Wang, C.X., Wang, L., Wang, L.Q., Wang, N.H., Wang, Q.L., Wang, S., Wang, X., Wang, Yu, Wang, Z.M., Wei, J., Weng, Z.L., Wu, H., Xiong, R.Q., Xu, W., Yan, Q., Yang, Y., Yashin, I.I., Yi, H., Yu, Y.M., Yu, Z.Q., Zannoni, M., Zhang, C., Zhang, F., Zhang, F.Z., Zhang, J.H., Zhang, Z., Zhao, F., Zheng, C., Zheng, Z.M., Zhuang, H.L., Zhukov, V., Zichichi, A., Zuccon, P., Demirköz, MELAHAT BİLGE, Sonnabend, R., Strigari, L., Su, T., Aguilar, M., Cavasonza, L. Ali, Ambrosi, G., Arruda, L., Attig, N., Barao, F., Barrin, L., Bartoloni, A., Basegmez-Du Pree, S., Battiston, R., Behlmann, M., Beranek, B., Berdugo, J., Bertucci, B., Bindi, V., Bollweg, K., Borgia, B., Boschini, M.J., Bourquin, M., Bueno, E.F., Burger, J., Burger, W.J., Burmeister, S., Cai, X.D., Capell, M., Casaus, J., Castellini, G., Cervelli, F., Chang, Y.H., Chen, G.M., Chen, G.R., Chen, H.S., Chen, Y., Cheng, L., Chou, H.Y., Chouridou, S., Choutko, V., Chung, C.H., Clark, C., Coignet, G., Consolandi, C., Contin, A., Corti, C., Cui, Z., Dadzie, K., Dass, A., Delgado, C., Della Torre, S., Derome, L., Di Falco, S., Di Felice, V., Díaz, C., Dimiccoli, F., Von Doetinchem, P., Dong, F., Donnini, F., Duranti, M., Egorov, A., Eline, A., Feng, J., Fiandrini, E., Fisher, P., Formato, V., Freeman, C., Gámez, C., García-López, R.J., Gargiulo, C., Gast, H., Gervasi, M., Giovacchini, F., Gómez-Coral, D.M., Gong, J., Goy, C., Grabski, V., Grandi, D., Graziani, M., Haino, S., Han, K.C., Hashmani, R.K., He, Z.H., Heber, B., Hsieh, T.H., Hu, J.Y., Incagli, M., Jang, W.Y., Jia, Yi, Jinchi, H., Karagöz, G., Khiali, B., Kim, G.N., Kirn, Th., Konyushikhin, M., Kounina, O., Kounine, A., Koutsenko, V., Krasnopevtsev, D., Kuhlman, A., Kulemzin, A., La Vacca, G., Laudi, E., Laurenti, G., Lazzizzera, I., Lebedev, A., Lee, H.T., Lee, S.C., Li, J.Q., Li, M., Li, Q., Li, S., Li, J.H., Li, Z.H., Liang, J., Light, C., Lin, C.H., Lippert, T., Liu, J.H., Liu, Z., Lu, S.Q., Lu, Y.S., Luebelsmeyer, K., Luo, J.Z., Luo, Xi, Machate, F., Mañá, C., Marín, J., Marquardt, J., Martin, T., Martínez, G., Masi, N., Maurin, D., Medvedeva, T., Menchaca-Rocha, A., Meng, Q., Mikhailov, V.V., Molero, M., Mott, P., Mussolin, L., Negrete, J., Nikonov, N., Nozzoli, F., Oliva, A., Orcinha, M., Palermo, M., Palmonari, F., Paniccia, M., Pashnin, A., Pauluzzi, M., Pensotti, S., Phan, H.D., Plyaskin, V., Pohl, M., Poluianov, S., Qin, X., Qu, Z.Y., Quadrani, L., Rancoita, P.G., Rapin, D., Conde, A. Reina, Robyn, E., Rosier-Lees, S., Rozhkov, A., Rozza, D., Sagdeev, R., Schael, S., Von Dratzig, A. Schultz, Schwering, G., Seo, E.S., Shakfa, Z., Shan, B.S., Siedenburg, T., Solano, C., Song, J.W., Song, X.J.

الوصف: We present the precision measurement of the daily proton fluxes in cosmic rays from May 20, 2011 to October 29, 2019 (a total of 2824 days or 114 Bartels rotations) in the rigidity interval from 1 to 100 GV based on 5.5 x 10(9) protons collected with the Alpha Magnetic Spectrometer aboard the International Space Station. The proton fluxes exhibit variations on multiple timescales. From 2014 to 2018, we observed recurrent flux variations with a period of 27 days. Shorter periods of 9 days and 13.5 days are observed in 2016. The strength of all three periodicities changes with time and rigidity. The rigidity dependence of the 27-day periodicity is different from the rigidity dependences of 9-day and 13.5-day periods. Unexpectedly, the strength of 9-day and 13.5-day periodicities increases with increasing rigidities up to similar to 10 GV and similar to 20 GV, respectively. Then the strength of the periodicities decreases with increasing rigidity up to 100 GV.

العلاقة: 8dc3fdd7-a65c-4b18-883e-e6315cb00dca; https://avesis.metu.edu.tr/publication/details/8dc3fdd7-a65c-4b18-883e-e6315cb00dca/oaiTest

الإتاحة: https://doi.org/10.1103/physrevlett.127.271102Test
https://avesis.metu.edu.tr/publication/details/8dc3fdd7-a65c-4b18-883e-e6315cb00dca/oaiTest

المؤلفون: Aguilar, M, Ambrosi, G, Anderson, H, Arruda, L, Attig, N, Bagwell, C, Barao, F, Barbanera, M, Barrin, L, Bartoloni, A, Battiston, R, Belyaev, N, Berdugo, J, Bertucci, B, Bindi, V, Bollweg, K, Bolster, J, Borchiellini, M, Borgia, B, Boschini, M.J, Bourquin, M, Burger, J, Burger, W.J, Cai, X.D, Capell, M, Casaus, J, Castellini, G, Cervelli, F, Chang, Y.H, Chen, G.M, Chen, G.R, Chen, H, Chen, H.S, Chen, Y, Cheng, L, Chou, H.Y, Chouridou, S, Choutko, V, Chung, C.H, Clark, C, Coignet, G, Consolandi, C, Contin, A, Corti, C, Cui, Z, Dadzie, K, d'Angelo, F, Dass, A, Delgado, C, Della Torre, S, Demirköz, M.B, Derome, L, Di Falco, S, Di Felice, V, Díaz, C, Dimiccoli, F, von Doetinchem, P, Dong, F, Donnini, F, Duranti, M, Egorov, A, Eline, A, Faldi, F, Feng, J, Fiandrini, E, Fisher, P, Formato, V, Gámez, C, García-López, R.J, Gargiulo, C, Gast, H, Gervasi, M, Giovacchini, F, Gómez-Coral, D.M, Gong, J, Goy, C, Grandi, D, Graziani, M, Guracho, A.N, Haino, S, Han, K.C, Hashmani, R.K, He, Z.H, Heber, B, Hsieh, T.H, Hu, J.Y, Huang, B.W, Ionica, M, Incagli, M, Jia, Yi, Jinchi, H, Karagöz, G, Khan, S, Khiali, B, Kirn, Th, Klipfel, A.P, Kounina, O, Kounine, A, Koutsenko, V, Krasnopevtsev, D, Kuhlman, A, Kulemzin, A, La Vacca, G, Laudi, E, Laurenti, G, Lavecchia, G, Lazzizzera, I, Lee, H.T, Lee, S.C, Li, H.L, Li, J.Q, Li, M, Li, Q, Li, Q.Y, Li, S, Li, S.L, Li, J.H, Li, Z.H, Liang, J, Liang, M.J, Lin, C.H, Lippert, T, Liu, J.H, Lu, S.Q, Lu, Y.S, Luebelsmeyer, K, Luo, J.Z, Luo, S.D, Luo, Xi, Mañá, C, Marín, J, Marquardt, J, Martin, T, Martínez, G, Masi, N, Maurin, D, Medvedeva, T, Menchaca-Rocha, A, Meng, Q, Molero, M, Mott, P, Mussolin, L, Jozani, Y. Najafi, Negrete, J, Nicolaidis, R, Nikonov, N, Nozzoli, F, Ocampo-Peleteiro, J, Oliva, A, Orcinha, M, Ottupara, M.A, Palermo, M, Palmonari, F, Paniccia, M, Pashnin, A, Pauluzzi, M, Pensotti, S, Plyaskin, V, Poluianov, S, Qin, X, Qu, Z.Y, Quadrani, L, Rancoita, P.G, Rapin, D, Conde, A. Reina, Robyn, E, Rodríguez-García, I, Romaneehsen, L, Rossi, F, Rozhkov, A, Rozza, D, Sagdeev, R, Savin, E, Schael, S, von Dratzig, A. Schultz, Schwering, G, Seo, E.S, Shan, B.S, Siedenburg, T, Silvestre, G, Song, J.W, Song, X.J, Sonnabend, R, Strigari, L, Su, T, Sun, Q, Sun, Z.T, Tacconi, M, Tang, X.W, Tang, Z.C, Tian, J, Tian, Y, Ting, Samuel C.C, Ting, S.M, Tomassetti, N, Torsti, J, Urban, T, Usoskin, I, Vagelli, V, Vainio, R, Valencia-Otero, M, Valente, E, Valtonen, E, Vázquez Acosta, M, Vecchi, M, Velasco, M, Vialle, J.P, Wang, C.X, Wang, L, Wang, L.Q, Wang, N.H, Wang, Q.L, Wang, S, Wang, X, Wang, Yu, Wang, Z.M, Wei, J, Weng, Z.L, Wu, H, Wu, Y, Xiao, J.N, Xiong, R.Q, Xiong, X.Z, Xu, W, Yan, Q, Yang, H.T, Yang, Y, Yelland, A, Yi, H, You, Y.H, Yu, Y.M, Yu, Z.Q, Zhang, C, Zhang, F, Zhang, F.Z, Zhang, J, Zhang, J.H, Zhang, Z, Zhao, F, Zheng, C, Zheng, Z.M, Zhuang, H.L, Zhukov, V, Zichichi, A, Zuccon, P

المساهمون: Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), AMS

المصدر: ISSN: 0031-9007.

مصطلحات موضوعية: positron, spectrum, cosmic radiation, galaxy, electron, AMS, satellite, magnetic spectrometer, solar, helium, structure, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]

الوصف: International audience ; We present the precision measurements of 11 years of daily cosmic positron fluxes in the rigidity range from 1.00 to 41.9 GV based on 3.4 × 10 6 positrons collected with the Alpha Magnetic Spectrometer (AMS) aboard the International Space Station. The positron fluxes show distinctly different time variations from the electron fluxes at short and long timescales. A hysteresis between the electron fluxes and the positron fluxes is observed with a significance greater than 5 σ at rigidities below 8.5 GV. On the contrary, the positron fluxes and the proton fluxes show similar time variation. Remarkably, we found that positron fluxes are modulated more than proton fluxes with a significance greater than 5 σ for rigidities below 7 GV. These continuous daily positron fluxes, together with AMS daily electron, proton, and helium fluxes over an 11-year solar cycle, provide unique input to the understanding of both the charge-sign and mass dependencies of cosmic rays in the heliosphere.

العلاقة: hal-04240476; https://hal.science/hal-04240476Test; INSPIRE: 2710091

الإتاحة: https://doi.org/10.1103/PhysRevLett.131.151002Test
https://hal.science/hal-04240476Test

المؤلفون: Aguilar, M, Cavasonza, L. Ali, Ambrosi, G, Arruda, L, Attig, N, Bagwell, C, Barao, F, Barrin, L, Bartoloni, A, Başeğmez-Du Pree, S, Battiston, R, Behlmann, M, Belyaev, N, Berdugo, J, Bertucci, B, Bindi, V, Bollweg, K, Bolster, J, Borgia, B, Boschini, M.J, Bourquin, M, Bueno, E.F, Burger, J, Burger, W.J, Burmeister, S, Cai, X.D, Capell, M, Casaus, J, Castellini, G, Cervelli, F, Chang, Y.H, Chen, G.M, Chen, G.R, Chen, H.S, Chen, Y, Cheng, L, Chou, H.Y, Chouridou, S, Choutko, V, Chung, C.H, Clark, C, Coignet, G, Consolandi, C, Contin, A, Corti, C, Cui, Z, Dadzie, K, Dass, A, Delgado, C, Della Torre, S, Demirköz, M.B, Derome, L, Di Falco, S, Di Felice, V, Díaz, C, Dimiccoli, F, von Doetinchem, P, Dong, F, Donnini, F, Duranti, M, Egorov, A, Eline, A, Faldi, F, Feng, J, Fiandrini, E, Fisher, P, Formato, V, Freeman, C, Gámez, C, García-López, R.J, Gargiulo, C, Gast, H, Gervasi, M, Giovacchini, F, Gómez-Coral, D.M, Gong, J, Goy, C, Grabski, V, Grandi, D, Graziani, M, Guracho, A.N, Haino, S, Han, K.C, Hashmani, R.K, He, Z.H, Heber, B, Hsieh, T.H, Hu, J.Y, Incagli, M, Jang, W.Y, Jia, Yi, Jinchi, H, Karagöz, G, Khiali, B, Kim, G.N, Kirn, Th, Kounina, O, Kounine, A, Koutsenko, V, Krasnopevtsev, D, Kuhlman, A, Kulemzin, A, La Vacca, G, Laudi, E, Laurenti, G, Lavecchia, G, Lazzizzera, I, Lee, H.T, Lee, S.C, Li, H.L, Li, J.Q, Li, M, Li, Q, Li, Q.Y, Li, S, Li, S.L, Li, J.H, Li, Z.H, Liang, J, Liang, M.J, Light, C, Lin, C.H, Lippert, T, Liu, J.H, Lu, S.Q, Lu, Y.S, Luebelsmeyer, K, Luo, J.Z, Luo, Xi, Machate, F, Mañá, C, Marín, J, Marquardt, J, Martin, T, Martínez, G, Masi, N, Maurin, D, Medvedeva, T, Menchaca-Rocha, A, Meng, Q, Mikhailov, V.V, Molero, M, Mott, P, Mussolin, L, Negrete, J, Nikonov, N, Nozzoli, F, Ocampo-Peleteiro, J, Oliva, A, Orcinha, M, Palermo, M, Palmonari, F, Paniccia, M, Pashnin, A, Pauluzzi, M, Pensotti, S, Plyaskin, V, Pohl, M, Poluianov, S, Qin, X, Qu, Z.Y, Quadrani, L, Rancoita, P.G, Rapin, D, Conde, A. Reina, Robyn, E, Rosier-Lees, S, Rozhkov, A, Rozza, D, Sagdeev, R, Schael, S, von Dratzig, A. Schultz, Schwering, G, Seo, E.S, Shan, B.S, Siedenburg, T, Song, J.W, Song, X.J, Sonnabend, R, Strigari, L, Su, T, Sun, Q, Sun, Z.T, Tacconi, M, Tang, X.W, Tang, Z.C, Tian, J, Ting, Samuel C.C, Ting, S.M, Tomassetti, N, Torsti, J, Urban, T, Usoskin, I, Vagelli, V, Vainio, R, Valencia-Otero, M, Valente, E, Valtonen, E, Vázquez Acosta, M, Vecchi, M, Velasco, M, Vialle, J.P, Wang, C.X, Wang, L, Wang, L.Q, Wang, N.H, Wang, Q.L, Wang, S, Wang, X, Wang, Yu, Wang, Z.M, Wei, J, Weng, Z.L, Wu, H, Xiong, R.Q, Xu, W, Yan, Q, Yang, Y, Yashin, I.I, Yelland, A, Yi, H, Yu, Y.M, Yu, Z.Q, Zannoni, M, Zhang, C, Zhang, F, Zhang, F.Z, Zhang, J.H, Zhang, Z, Zhao, F, Zheng, C, Zheng, Z.M, Zhuang, H.L, Zhukov, V, Zichichi, A, Zuccon, P

المساهمون: Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), AMS

المصدر: ISSN: 0031-9007.

مصطلحات موضوعية: electron, flux, cosmic radiation, galaxy, spectrum, structure, satellite, magnetic spectrometer, electron p, solar, AMS, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]

الوصف: International audience ; We present the precision measurements of 11 years of daily cosmic electron fluxes in the rigidity interval from 1.00 to 41.9 GV based on 2.0 × 10 8 electrons collected with the Alpha Magnetic Spectrometer (AMS) aboard the International Space Station. The electron fluxes exhibit variations on multiple timescales. Recurrent electron flux variations with periods of 27 days, 13.5 days, and 9 days are observed. We find that the electron fluxes show distinctly different time variations from the proton fluxes. Remarkably, a hysteresis between the electron flux and the proton flux is observed with a significance of greater than 6 σ at rigidities below 8.5 GV. Furthermore, significant structures in the electron-proton hysteresis are observed corresponding to sharp structures in both fluxes. This continuous daily electron data provide unique input to the understanding of the charge sign dependence of cosmic rays over an 11-year solar cycle.

العلاقة: hal-04074601; https://hal.science/hal-04074601Test; INSPIRE: 2651726

الإتاحة: https://doi.org/10.1103/PhysRevLett.130.161001Test
https://hal.science/hal-04074601Test

المؤلفون: Aguilar, M, Ali Cavasonza, L, Alpat, B, Ambrosi, G, Arruda, L, Attig, N, Bagwell, C, Barao, F, Barrin, L, Bartoloni, A, Başeğmez-Du Pree, S, Battiston, R, Belyaev, N, Berdugo, J, Bertucci, B, Bindi, V, Bollweg, K, Bolster, J, Borchiellini, M, Borgia, B, Boschini, M.J, Bourquin, M, Bueno, E.F, Burger, J, Burger, W.J, Cai, X.D, Capell, M, Casaus, J, Castellini, G, Cervelli, F, Chang, Y.H, Chen, G.M, Chen, G.R, Chen, H, Chen, H.S, Chen, Y, Cheng, L, Chou, H.Y, Chouridou, S, Choutko, V, Chung, C.H, Clark, C, Coignet, G, Consolandi, C, Contin, A, Corti, C, Cui, Z, Dadzie, K, Dass, A, Delgado, C, Della Torre, S, Demirköz, M.B, Derome, L, Di Falco, S, Di Felice, V, Díaz, C, Dimiccoli, F, von Doetinchem, P, Dong, F, Donnini, F, Duranti, M, Egorov, A, Eline, A, Faldi, F, Feng, J, Fiandrini, E, Fisher, P, Formato, V, Gámez, C, García-López, R.J, Gargiulo, C, Gast, H, Gervasi, M, Giovacchini, F, Gómez-Coral, D.M, Gong, J, Goy, C, Grabski, V, Grandi, D, Graziani, M, Guracho, A.N, Haino, S, Han, K.C, Hashmani, R.K, He, Z.H, Heber, B, Hsieh, T.H, Hu, J.Y, Huang, B.W, Incagli, M, Jang, W.Y, Jia, Yi, Jinchi, H, Karagöz, G, Khiali, B, Kim, G.N, Kirn, Th, Kounina, O, Kounine, A, Koutsenko, V, Krasnopevtsev, D, Kuhlman, A, Kulemzin, A, La Vacca, G, Laudi, E, Laurenti, G, Lavecchia, G, Lazzizzera, I, Lee, H.T, Lee, S.C, Li, H.L, Li, J.Q, Li, M, Li, Q, Li, Q.Y, Li, S, Li, S.L, Li, J.H, Li, Z.H, Liang, J, Liang, M.J, Lin, C.H, Lippert, T, Liu, J.H, Lu, S.Q, Lu, Y.S, Luebelsmeyer, K, Luo, J.Z, Luo, S.D, Luo, Xi, Machate, F, Mañá, C, Marín, J, Marquardt, J, Martin, T, Martínez, G, Masi, N, Maurin, D, Medvedeva, T, Menchaca-Rocha, A, Meng, Q, Mikhailov, V.V, Molero, M, Mott, P, Mussolin, L, Negrete, J, Nikonov, N, Nozzoli, F, Ocampo-Peleteiro, J, Oliva, A, Orcinha, M, Ottupara, M.A, Palermo, M, Palmonari, F, Paniccia, M, Pashnin, A, Pauluzzi, M, Pensotti, S, Plyaskin, V, Poluianov, S, Qin, X, Qu, Z.Y, Quadrani, L, Rancoita, P.G, Rapin, D, Reina Conde, A, Robyn, E, Romaneehsen, L, Rozhkov, A, Rozza, D, Sagdeev, R, Schael, S, Schultz von Dratzig, A, Schwering, G, Seo, E.S, Shan, B.S, Siedenburg, T, Song, J.W, Song, X.J, Sonnabend, R, Strigari, L, Su, T, Sun, Q, Sun, Z.T, Tacconi, M, Tang, X.W, Tang, Z.C, Tian, J, Tian, Y, Ting, Samuel C.C, Ting, S.M, Tomassetti, N, Torsti, J, Urban, T, Usoskin, I, Vagelli, V, Vainio, R, Valencia-Otero, M, Valente, E, Valtonen, E, Vázquez Acosta, M, Vecchi, M, Velasco, M, Vialle, J.P, Wang, C.X, Wang, L, Wang, L.Q, Wang, N.H, Wang, Q.L, Wang, S, Wang, X, Wang, Yu, Wang, Z.M, Wei, J, Weng, Z.L, Wu, H, Wu, Y, Xiao, J.N, Xiong, R.Q, Xiong, X.Z, Xu, W, Yan, Q, Yang, H.T, Yang, Y, Yashin, I.I, Yelland, A, Yi, H, You, Y.H, Yu, Y.M, Yu, Z.Q, Zannoni, M, Zhang, C, Zhang, F, Zhang, F.Z, Zhang, J, Zhang, J.H, Zhang, Z, Zhao, F, Zheng, C, Zheng, Z.M, Zhuang, H.L, Zhukov, V, Zichichi, A, Zuccon, P

المساهمون: Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), AMS

المصدر: ISSN: 0031-9007.

مصطلحات موضوعية: cosmic radiation, primary, boron, flux, carbon, oxygen, propagation, sulfur, magnetic spectrometer, neon, silicon, nucleus, magnesium, AMS, fluorine, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]

الوصف: International audience ; We report the properties of primary cosmic-ray sulfur (S) in the rigidity range 2.15 GV to 3.0 TV based on 0.38 × 10 6 sulfur nuclei collected by the Alpha Magnetic Spectrometer experiment (AMS). We observed that above 90 GV the rigidity dependence of the S flux is identical to the rigidity dependence of Ne-Mg-Si fluxes, which is different from the rigidity dependence of the He-C-O-Fe fluxes. We found that, similar to N, Na, and Al cosmic rays, over the entire rigidity range, the traditional primary cosmic rays S, Ne, Mg, and C all have sizeable secondary components, and the S, Ne, and Mg fluxes are well described by the weighted sum of the primary silicon flux and the secondary fluorine flux, and the C flux is well described by the weighted sum of the primary oxygen flux and the secondary boron flux. The primary and secondary contributions of the traditional primary cosmic-ray fluxes of C, Ne, Mg, and S (even Z elements) are distinctly different from the primary and secondary contributions of the N, Na, and Al (odd Z elements) fluxes. The abundance ratio at the source for S / Si is 0.167 ± 0.006 , for Ne / Si is 0.833 ± 0.025 , for Mg / Si is 0.994 ± 0.029 , and for C / O is 0.836 ± 0.025 . These values are determined independent of cosmic-ray propagation.

العلاقة: hal-04107906; https://hal.science/hal-04107906Test; INSPIRE: 2662857

الإتاحة: https://doi.org/10.1103/PhysRevLett.130.211002Test
https://hal.science/hal-04107906Test

المؤلفون: Zhang, J.H., Demirköz, MELAHAT BİLGE, Zuccon, P., Zichichi, A., Zhukov, V., Zhuang, H.L., Zheng, Z.M., Zheng, C., Zhao, F., Zhang, Z., Zhang, F.Z., Zhang, F., Zhang, C., Zannoni, M., Yu, Z.Q., Yu, Y.M., Yi, H., Yelland, A., Yashin, I.I., Yang, Y., Yan, Q., Xu, W., Xiong, R.Q., Wu, H., Weng, Z.L., Wei, J., Wang, Z.M., Wang, Yu, Wang, X., Wang, S., Wang, Q.L., Wang, N.H., Wang, L.Q., Wang, L., Wang, C.X., Vialle, J.P., Velasco, M., Vecchi, M., Vázquez Acosta, M., Valtonen, E., Valente, E., Valencia-Otero, M., Vainio, R., Vagelli, V., Usoskin, I., Urban, T., Torsti, J., Tomassetti, N., Ting, S.M., Ting, Samuel C. C., Tian, J., Tang, Z.C., Tang, X.W., Tacconi, M., Sun, Z.T., Sun, Q., Su, T., Strigari, L., Sonnabend, R., Song, X.J., Song, J.W., Siedenburg, T., Shan, B.S., Seo, E.S., Schwering, G., Von Dratzig, A. Schultz, Schael, S., Sagdeev, R., Rozza, D., Rozhkov, A., Rosier-Lees, S., Robyn, E., Conde, A. Reina, Rapin, D., Rancoita, P.G., Quadrani, L., Qu, Z.Y., Qin, X., Poluianov, S., Pohl, M., Plyaskin, V., Pensotti, S., Pauluzzi, M., Pashnin, A., Paniccia, M., Palmonari, F., Palermo, M., Orcinha, M., Oliva, A., Ocampo-Peleteiro, J., Nozzoli, F., Nikonov, N., Negrete, J., Mussolin, L., Mott, P., Molero, M., Mikhailov, V.V., Meng, Q., Menchaca-Rocha, A., Medvedeva, T., Maurin, D., Masi, N., Martínez, G., Martin, T., Marquardt, J., Marín, J., Mañá, C., MacHate, F., Luo, Xi, Luo, J.Z., Luebelsmeyer, K., Lu, Y.S., Lu, S.Q., Liu, J.H., Lippert, T., Lin, C.H., Light, C., Liang, M.J., Liang, J., Li, Z.H., Li, J.H., Li, S.L., Li, S., Li, Q.Y., Li, Q., Li, M., Li, J.Q., Li, H.L., Lee, S.C., Lee, H.T., Lazzizzera, I., Lavecchia, G., Laurenti, G., Laudi, E., La Vacca, G., Kulemzin, A., Kuhlman, A., Krasnopevtsev, D., Koutsenko, V., Kounine, A., Kounina, O., Kirn, Th., Kim, G.N., Khiali, B., Karagöz, G., Jinchi, H., Jia, Yi, Jang, W.Y., Incagli, M., Hu, J.Y., Hsieh, T.H., Heber, B., He, Z.H., Hashmani, R.K., Han, K.C., Haino, S., Guracho, A.N., Graziani, M., Grandi, D., Grabski, V., Goy, C., Gong, J., Gómez-Coral, D.M., Giovacchini, F., Gervasi, M., Gast, H., Gargiulo, C., García-López, R.J., Gámez, C., Freeman, C., Formato, V., Fisher, P., Fiandrini, E., Feng, J., Faldi, F., Eline, A., Egorov, A., Duranti, M., Donnini, F., Dong, F., Von Doetinchem, P., Dimiccoli, F., Díaz, C., Di Felice, V., Di Falco, S., Derome, L., Della Torre, S., Delgado, C., Dass, A., Dadzie, K., Cui, Z., Corti, C., Contin, A., Consolandi, C., Coignet, G., Clark, C., Chung, C.H., Choutko, V., Chouridou, S., Chou, H.Y., Cheng, L., Chen, Y., Chen, H.S., Chen, G.R., Chen, G.M., Chang, Y.H., Cervelli, F., Castellini, G., Casaus, J., Capell, M., Cai, X.D., Burmeister, S., Burger, W.J., Burger, J., Bueno, E.F., Bourquin, M., Boschini, M.J., Borgia, B., Bolster, J., Bollweg, K., Bindi, V., Bertucci, B., Berdugo, J., Belyaev, N., Behlmann, M., Battiston, R., Başeǧmez-Du Pree, S., Bartoloni, A., Barrin, L., Barao, F., Bagwell, C., Attig, N., Arruda, L., Ambrosi, G., Cavasonza, L. Ali, Aguilar, M.

الوصف: We present the precision measurements of 11 years of daily cosmic electron fluxes in the rigidity interval from 1.00 to 41.9 GV based on 2.0 x 108 electrons collected with the Alpha Magnetic Spectrometer (AMS) aboard the International Space Station. The electron fluxes exhibit variations on multiple timescales. Recurrent electron flux variations with periods of 27 days, 13.5 days, and 9 days are observed. We find that the electron fluxes show distinctly different time variations from the proton fluxes. Remarkably, a hysteresis between the electron flux and the proton flux is observed with a significance of greater than 6 sigma at rigidities below 8.5 GV. Furthermore, significant structures in the electron-proton hysteresis are observed corresponding to sharp structures in both fluxes. This continuous daily electron data provide unique input to the understanding of the charge sign dependence of cosmic rays over an 11-year solar cycle.

العلاقة: c8102bd2-c792-4982-853b-875b2bb86999; https://avesis.metu.edu.tr/publication/details/c8102bd2-c792-4982-853b-875b2bb86999/oaiTest

الإتاحة: https://doi.org/10.1103/physrevlett.130.161001Test
https://avesis.metu.edu.tr/publication/details/c8102bd2-c792-4982-853b-875b2bb86999/oaiTest