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  1. Book ; Online: Feasibility study to characterize the production of antineutrons in high energy $pp$ collisions through charge exchange interactions

    Lugo-Porras, F. / Gomez-Coral, D. M. / Menchaca-Rocha, A.

    2023  

    Abstract: Simulations to evaluate the feasibility of $\bar{n}$ identification and kinematic characterization via the hadronic charge exchange (CEX) interaction $n+\bar{n}\rightarrow p+\bar{p}$ are reported. The target neutrons are those composing the silicon ... ...

    Abstract Simulations to evaluate the feasibility of $\bar{n}$ identification and kinematic characterization via the hadronic charge exchange (CEX) interaction $n+\bar{n}\rightarrow p+\bar{p}$ are reported. The target neutrons are those composing the silicon nuclei of which inner tracking devices present in LHC experiments are made. Simulations of $pp$ collisions in PYTHIA were carried out at different energies to investigate $\bar{n}$ production and the expected $\bar{n}$ energy spectra. Then, two types of GEANT4 simulations were performed, placing an $\bar{n}$ point source at the ALICE primary vertex as a working example. In the first simulation, the $E_k$ was kept at an arbitrary (1 GeV) fix value to develop an $\bar{n}$ identification and kinematics reconstruction protocol. The second GEANT4 simulation used the resulting PYTHIA at $\sqrt{s_{pp}}=13$ TeV $\bar{n}$ energy spectra. In both simulations, the occurrence of CEX interactions was identified by the unique outgoing $\bar{p}$. The simplified simulation allowed to estimate a 0.11% CEX-interaction identification efficiency at $E_k = 1$ GeV. The $p$ CEX-partner identification is challenging because of the presence of silicon nucleus-fragmentation protons. Momentum correlations between the $\bar{n}$ and all possible $\bar{p}p$ pairs showed that $p$ CEX-partner identification and $\bar{n}$ kinematics reconstruction corresponds to minimal momentum-loss events. The use of ITS $dE/dx$ information is found to improve $\bar{n}$ identification and kinematic characterization in both simulations. The final protocol applied to the realistic simulation resulted in a $\bar{n}$ identification and kinematic reconstruction efficiency of 0.006%, based solely on $\bar{p}p $ pair observable. Thus, the expected rate of identified and kinematically reconstructed $\bar{n}$ should lie in the order of 100,000 per second, illustrating the feasibility of the method.

    Comment: 6 pages, 11 figures
    Keywords High Energy Physics - Experiment
    Subject code 660
    Publishing date 2023-09-13
    Publishing country us
    Document type Book ; Online
    Database BASE - Bielefeld Academic Search Engine (life sciences selection)

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  2. Article: Science and technology in Mexico.

    Menchaca-Rocha, Arturo

    Nature materials

    2010  Volume 9, Issue 10, Page(s) 781–783

    Language English
    Publishing date 2010-09-15
    Publishing country England
    Document type Journal Article
    ZDB-ID 2088679-2
    ISSN 1476-4660 ; 1476-1122
    ISSN (online) 1476-4660
    ISSN 1476-1122
    DOI 10.1038/nmat2869
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  3. Book ; Online: Prototype-module of a muon tracker to investigate the Popocatepetl volcano lava dome density-distribution

    Grabski, V. / Velázquez-Carreón, F. / Aguilar, S. / Menchaca-Rocha, A. / Urrutia-Fucugauchi, J. / Zmeskal, J.

    2019  

    Abstract: The study of volcanic inner density distributions using cosmic muons is an innovative method, which is still in a stage of development. This technique can be used to determine the average density along the muon track, as well as the density distribution ... ...

    Abstract The study of volcanic inner density distributions using cosmic muons is an innovative method, which is still in a stage of development. This technique can be used to determine the average density along the muon track, as well as the density distribution within a given volume, by measuring the attenuation of the cosmic muon flux going through it. The aim is to study the volcano domes and magmatic conduit systems within a given time-interval. Our first application will be the Popocatepetl, a large active andesitic stratovolcano built in the Trans-Mexican volcanic arc. Its recent activity includes emplacement of a lava dome, with explosions and frequent scoria and ash emissions. This study is part of a longer-term project of volcanic hazard monitoring that includes other Mexican volcanoes, like the Colima. Muon detector design depends on the volume-of-interest dimensions, as well as on the image-taking frequency required to detect dynamic density variations. Our muon-tracker proposal includes 3 planes, each having 16 independent position-sensitive modules consisting on rectangular aluminum tubes ($10x20x320cm^{3}$) filed with a liquid scintillator. The light collection inside each module is carried out using a wave-length-shifting (WLS) fiber matrix, running along the aluminum-tube length, which is bundled together at the tube extremes. The luminous signal readout is carried out using one SiPM optically coupled to the WLS bundle at each modules end. The main detector characteristics, such as time resolution, surface uniformity, and signal amplitude reconstruction using the time-over-threshold technique, will be presented.
    Keywords Physics - Instrumentation and Detectors ; High Energy Physics - Experiment
    Subject code 621
    Publishing date 2019-08-31
    Publishing country us
    Document type Book ; Online
    Database BASE - Bielefeld Academic Search Engine (life sciences selection)

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  4. Article: Coalescence of liquid drops by surface tension.

    Menchaca-Rocha, A / Martínez-Dávalos, A / Núñez, R / Popinet, S / Zaleski, S

    Physical review. E, Statistical, nonlinear, and soft matter physics

    2001  Volume 63, Issue 4 Pt 2, Page(s) 46309

    Abstract: The merging of two mercury drops at very low kinetic energy is observed using fast, digital, and analog imaging techniques. Sequences showing the time evolution of the overall-surface shape as well as an amplified view of the contact region are shown. ... ...

    Abstract The merging of two mercury drops at very low kinetic energy is observed using fast, digital, and analog imaging techniques. Sequences showing the time evolution of the overall-surface shape as well as an amplified view of the contact region are shown. Qualitative and quantitative comparisons with computations of the Navier-Stokes equation with a free surface are made. In the model, the surface is tracked by a marker-chain method.
    Language English
    Publishing date 2001-04
    Publishing country United States
    Document type Journal Article
    ISSN 1539-3755
    ISSN 1539-3755
    DOI 10.1103/PhysRevE.63.046309
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  5. Article: Model of ion-induced luminescence based on energy deposition by secondary electrons.

    Michaelian / Menchaca-Rocha

    Physical review. B, Condensed matter

    1994  Volume 49, Issue 22, Page(s) 15550–15562

    Language English
    Publishing date 1994-06-01
    Publishing country United States
    Document type Journal Article
    ZDB-ID 209770-9
    ISSN 1095-3795 ; 1550-235X ; 0163-1829 ; 2469-9950 ; 1098-0121 ; 0556-2805
    ISSN (online) 1095-3795 ; 1550-235X
    ISSN 0163-1829 ; 2469-9950 ; 1098-0121 ; 0556-2805
    DOI 10.1103/physrevb.49.15550
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  6. Article: Rotating-liquid-drop model limit tested on macroscopic drops.

    Menchaca-Rocha / Cuevas / Chapa / Silva

    Physical review. E, Statistical physics, plasmas, fluids, and related interdisciplinary topics

    1993  Volume 47, Issue 2, Page(s) 1433–1436

    Language English
    Publishing date 1993-02
    Publishing country United States
    Document type Journal Article
    ISSN 1063-651X
    ISSN 1063-651X
    DOI 10.1103/physreve.47.1433
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  7. Article ; Online: Temporal Structures in Positron Spectra and Charge-Sign Effects in Galactic Cosmic Rays.

    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

    Physical review letters

    2023  Volume 131, Issue 15, Page(s) 151002

    Abstract: 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 ... ...

    Abstract 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 5σ 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 5σ 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.
    Language English
    Publishing date 2023-10-28
    Publishing country United States
    Document type Journal Article
    ZDB-ID 208853-8
    ISSN 1079-7114 ; 0031-9007
    ISSN (online) 1079-7114
    ISSN 0031-9007
    DOI 10.1103/PhysRevLett.131.151002
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  8. Article ; Online: Properties of Cosmic-Ray Sulfur and Determination of the Composition of Primary Cosmic-Ray Carbon, Neon, Magnesium, and Sulfur: Ten-Year Results from the Alpha Magnetic Spectrometer.

    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

    Physical review letters

    2023  Volume 130, Issue 21, Page(s) 211002

    Abstract: 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 ... ...

    Abstract 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.
    MeSH term(s) Magnesium ; Neon ; Carbon ; Sulfur ; Magnetic Phenomena
    Chemical Substances Magnesium (I38ZP9992A) ; Neon (4VB4Y46AHD) ; Carbon (7440-44-0) ; Sulfur (70FD1KFU70)
    Language English
    Publishing date 2023-05-26
    Publishing country United States
    Document type Journal Article
    ZDB-ID 208853-8
    ISSN 1079-7114 ; 0031-9007
    ISSN (online) 1079-7114
    ISSN 0031-9007
    DOI 10.1103/PhysRevLett.130.211002
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  9. Article ; Online: Temporal Structures in Electron Spectra and Charge Sign Effects in Galactic Cosmic Rays.

    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

    Physical review letters

    2023  Volume 130, Issue 16, Page(s) 161001

    Abstract: 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 ...

    Abstract 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 6σ 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.
    Language English
    Publishing date 2023-05-08
    Publishing country United States
    Document type Journal Article
    ZDB-ID 208853-8
    ISSN 1079-7114 ; 0031-9007
    ISSN (online) 1079-7114
    ISSN 0031-9007
    DOI 10.1103/PhysRevLett.130.161001
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  10. Article ; Online: Periodicities in the Daily Proton Fluxes from 2011 to 2019 Measured by the Alpha Magnetic Spectrometer on the International Space Station from 1 to 100 GV.

    Aguilar, M / Cavasonza, L Ali / Ambrosi, G / Arruda, L / Attig, N / Barao, F / Barrin, L / Bartoloni, A / Başeğmez-du Pree, S / Battiston, R / Behlmann, M / Beranek, B / Berdugo, J / Bertucci, B / Bindi, V / Bollweg, K / Borgia, B / Boschini, M J / Bourquin, M /
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    Physical review letters

    2022  Volume 127, Issue 27, Page(s) 271102

    Abstract: 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 5.5×10^{9} protons collected with the ... ...

    Abstract 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 5.5×10^{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 ∼10  GV and ∼20  GV, respectively. Then the strength of the periodicities decreases with increasing rigidity up to 100 GV.
    Language English
    Publishing date 2022-01-21
    Publishing country United States
    Document type Journal Article
    ZDB-ID 208853-8
    ISSN 1079-7114 ; 0031-9007
    ISSN (online) 1079-7114
    ISSN 0031-9007
    DOI 10.1103/PhysRevLett.127.271102
    Database MEDical Literature Analysis and Retrieval System OnLINE

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