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Observation of Fine Time Structures in the Cosmic Proton and Helium Fluxes with the Alpha Magnetic Spectrometer on the International Space Station

2018· article· en· W2885695515 on OpenAlexfundno aff
M. Aguilar, L. Ali Cavasonza, B. Alpat, G. Ambrosi, L. Arruda, N. Attig, S. Aupetit, P. Azzarello, A. Bachlechner, F. Barão, Aurélien Barrau, L. Barrin, A. Bartoloni, L. Basara, Seth Pree, Markus Battarbee, R. Battiston, U. Becker, M. Behlmann, B. Beischer, J. Berdugo, B. Bertucci, K. F. Bindel, V. Bindi, W. De Boer, K. Bollweg, V. Bonnivard, B. Borgia, M. Boschini, M. Bourquin, E. F. Bueno, Johanna Bürger, F. Cadoux, Xudong Cai, M. Capell, Sami Caroff, J. Casaus, G. Castellini, F. Cervelli, M. J. Chae, Y. H. Chang, A. I. Chen, G. M. Chen, H. S. Chen, Y. Chen, Lin Cheng, H. Y. Chou, E. Choumilov, V. Choutko, C. H. Chung, C. Clark, R. Clavero, G. Coignet, C. Consolandi, A. Contin, C. Corti, W. Creus, M. Crispoltoni, Z. Cui, S. Kokou Dadzie, Ye Dai, A. Datta, S. Della Torre, B. Demirköz, L. Derome, S. Di Falco, F. Dimiccoli, C. Díaz, P. von Doetinchem, Fang Dong, F. Donnini, M. Duranti, D. D’Urso, A. I. Egorov, A. Eline, T. Eronen, J. H. Feng, E. Fiandrini, P.H. Fisher, V. Formato, Yu. Galaktionov, G. Gallucci, R. J. Garcı́a López, Corrado Gargiulo, H. Gast, Iris Gebauer, M. Gervasi, A. Ghelfi, F. Giovacchini, D. M. Gómez-Coral, J. Gong, C. Goy, Varlen Grabski, D. Grandi, M. Graziani, K. H. Guo, S. Haino, K. C. Han, Z. H. He, M. Heil, J. Hoffman, Timothy H. Hsieh, H. Huang, Z. C. Huang, C. Huh, M. Incagli, M. Ionica, W. Jang, Yi Jia, H. Jinchi, S. C. Kang, K. Kanishev, B. Khiali, G. N. Kim, K. S. Kim, Th. Kirn, O. Kounina, A. Kounine, V. Koutsenko, A. Kulemzin, G. La Vacca, E. Laudi, G. Laurenti, I. Lazzizzera, A. Lebedev, H. T. Lee, S. C. Lee, C. Leluc, H. S. Li, Qiang Li, Q. Li, T. X. Li, Z. H. Li, Z. Y. Li, Christopher Light, Soobin Lim, Chao‐Hung Lin, P. Lipari, Thomas Lippert, D. Liu, Hu Liu, V. D. Lordello, S. Q. Lu, Yudong Lu, K. Luebelsmeyer, Feng Luo, Junzhou Luo, Xi Luo, Shaoyu Lyu, F. Machate, C. Mañá, J. Marín, T. Martin, G. Martı́nez, N. Masi, D. Maurin, A. Menchaca-Rocha, Q. Meng, V. M. Mikuni, Dong-Chuan Mo, P. Mott, T. Nelson, J. Q. Ni, N. Nikonov, F. Nozzoli, A. Oliva, M. Orcinha, M. Palermo, F. Palmonari, C. Palomares, M. Paniccia, M. Pauluzzi, S. Pensotti, C. Perrina, H. D. Phan, N. Picot-Clémente, F. Pilo, C. Pizzolotto, V. Plyaskin, M. Pohl, V. Poireau, A. Popkow, L. Quadrani, X. M. Qi, X. Qin, Z. Y. Qu, T. Räihä, P.G. Rancoita, D. Rapin, J. S. Ricol, S. Rosier-Lees, A. Rozhkov, D. Rozza, R. Z. Sagdeev, S. Schael, Susann Schmidt, A. Schulz von Dratzig, G. Schwering, E. S. Seo, B. S. Shan, J. Y. Shi, T. Siedenburg, D. Son, Jiwei Song, M. Tacconi, Xiao Tang, Zhi-Cheng Tang, D. Tescaro, Samuel C.C. Ting, S.M. Ting, Nicola Tomassetti, J. Torsti, C. Türkoğlu, T. Urban, V. Vagelli, E. Valente, E. Valtonen, M. Vázquez Acosta, M. Vecchi, M. Velasco, J. P. Vialle, L. Q. Wang, H. Wang, Qiuliang Wang, X. Wang, X. Q. Wang, Z. X. Wang, Chuncheng Wei, Z. Weng, Kathryn Whitman, H. Wu, X. Wu, R. Q. Xiong, W. Xu, Qi Yan, J. Yang, Min Yang, Y. Yang, Han Yi, Yaxin Yu, Z. Q. Yu, M. Zannoni, S. Zeissler, C. Zhang, F. Zhang, J. Zhang, J. H. Zhang, S. W. Zhang, Z. Zhang, Z. M. Zheng, H. L. Zhuang, V. Zhukov, A. Zichichi, N. Zimmermann, P. Zuccon

Bibliographic record

VenuePhysical Review Letters · 2018
Typearticle
Languageen
FieldPhysics and Astronomy
TopicSolar and Space Plasma Dynamics
Canadian institutionsnot available
FundersCentro de Investigaciones Energéticas, Medioambientales y TecnológicasSecretaría de Estado de Investigación, Desarrollo e InnovaciónInstitut National de Physique Nucléaire et de Physique des ParticulesHorizon 2020 Framework ProgrammeArgonne National LaboratoryJohnson Space CenterMarshall Space Flight CenterProducteurs d'oeufs d'incubation du CanadaUniversidad Nacional Autónoma de MéxicoCentre National de la Recherche ScientifiqueMinistry of Science and Technology, TaiwanNatural Science Foundation of Shandong ProvinceChina Scholarship CouncilNational Research Foundation of KoreaTekesH2020 Marie Skłodowska-Curie ActionsStrongSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungDeutsches Zentrum für Luft- und RaumfahrtFundação para a Ciência e a TecnologiaChinese Academy of SciencesCentre National d’Etudes SpatialesMinistry of Science and Technology of the People's Republic of ChinaEwha Womans UniversityAcademy of FinlandU.S. Department of EnergyNational Natural Science Foundation of ChinaFundação de Amparo à Pesquisa do Estado de São PauloCentro para el Desarrollo Tecnológico IndustrialAcademia SinicaInstituto Nazionale di Fisica NucleareMassachusetts Institute of TechnologyEuropean CommissionAgenzia Spaziale ItalianaNational Energy Research Scientific Computing CenterCERNKyungpook National UniversityAgence Nationale de la RechercheNational Science FoundationEuropean Space AgencyNational Aeronautics and Space AdministrationConsejo Nacional de Ciencia y TecnologíaTürkiye Atom Enerjisi Kurumu
KeywordsPhysicsHeliumAmplitudeCosmic rayFlux (metallurgy)ProtonSpectrometerSolar maximumRigidity (electromagnetism)Isotopes of heliumSolar minimumInternational Space StationNuclear physicsSolar cycleAtomic physicsAstrophysicsSolar windPlasmaAstronomyOptics

Abstract

fetched live from OpenAlex

We present the precision measurement from May 2011 to May 2017 (79 Bartels rotations) of the proton fluxes at rigidities from 1 to 60 GV and the helium fluxes from 1.9 to 60 GV based on a total of 1×10^{9} events collected with the Alpha Magnetic Spectrometer aboard the International Space Station. This measurement is in solar cycle 24, which has the solar maximum in April 2014. We observed that, below 40 GV, the proton flux and the helium flux show nearly identical fine structures in both time and relative amplitude. The amplitudes of the flux structures decrease with increasing rigidity and vanish above 40 GV. The amplitudes of the structures are reduced during the time period, which started one year after solar maximum, when the proton and helium fluxes steadily increase. Above ∼3 GV the p/He flux ratio is time independent. We observed that below ∼3 GV the ratio has a long-term decrease coinciding with the period during which the fluxes start to rise.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.003
Threshold uncertainty score0.005

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0020.001
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.009
GPT teacher head0.244
Teacher spread0.235 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

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Citations149
Published2018
Admission routes1
Has abstractyes

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