H. L. Li
Academia Sinica
5 Papers
4 Citations
H. L. Li is an academic researcher from Academia Sinica. The author has contributed to research in topics: Cosmic ray & Stars. The author has an hindex of 2, co-authored 2 publications.
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Papers
Precision Measurement of the Proton Flux in Primary Cosmic Rays from Rigidity 1 GV to 1.8 TV with the Alpha Magnetic Spectrometer on the International Space Station
M. Aguilar,D. Aisa,Behcet Alpat,A. Alvino,G. Ambrosi,K. Andeen,Luísa Arruda,N. Attig,Philipp Azzarello,A. Bachlechner,Fernando Barão,A. Barrau,L. Barrin,A. Bartoloni,L. Basara,Markus Battarbee,Roberto Battiston,J. Bazo,U. Becker,M. Behlmann,B. Beischer,J. Berdugo,B. Bertucci,G. Bigongiari,Veronica Bindi,S. Bizzaglia,M. Bizzarri,G. Boella,W. De Boer,K. Bollweg,V. Bonnivard,B. Borgia,S. Borsini,Matteo Boschini,M. Bourquin,J. D. Burger,Franck Cadoux,X. D. Cai,M. Capell,S. Caroff,J. Casaus,V. Cascioli,G. Castellini,I. Cernuda,D. Cerreta,F. Cervelli,M. J. Chae,Yuan-Hann Chang,A. I. Chen,H. S. Chen,G. M. Cheng,H. S. Chen,Lin Cheng,H. Y. Chou,E. Choumilov,V. Choutko,C. H. Chung,C. Clark,R. Clavero,G. Coignet,C. Consolandi,A. Contin,Claudio Corti,E. Cortina Gil,B. Coste,W. Creus,M. Crispoltoni,Z. Cui,Yaomin Dai,C. Delgado,S. Della Torre,M. B. Demirköz,Laurent Derome,S. Di Falco,L. Di Masso,F. Dimiccoli,Carlos Díaz,P. von Doetinchem,F. Donnini,W. J. Du,M. Duranti,D. D'Urso,A. Eline,F. J. Eppling,T. Eronen,Y. Y. Fan,L. Farnesini,J. Feng,E. Fiandrini,A. Fiasson,E. Finch,Peter H. Fisher,Yu. Galaktionov,G. Gallucci,Bruce Rafael Mellado Garcia,R. J. García-López,Corrado Gargiulo,Henning Gast,I. Gebauer,Massimo Gervasi,A. Ghelfi,W. Gillard,F. Giovacchini,P. Goglov,J. Gong,C. Goy,Varlen Grabski,D. Grandi,M. Graziani,C. Guandalini,I. Guerri,K. H. Guo,D. Haas,M. Habiby,Sadakazu Haino,K. C. Han,Z. H. He,Matthias Heil,J. Hoffman,Timothy H. Hsieh,Zhiqi Huang,Changgi Huh,M. Incagli,Maria Ionica,W. Y. Jang,H. Jinchi,K. Kanishev,G. N. Kim,Kwangsoo Kim,T. Kirn,R. Kossakowski,O. Kounina,Andrei Kounine,V. Koutsenko,M. S. Krafczyk,G. La Vacca,E. Laudi,G. Laurenti,I. Lazzizzera,A. Lebedev,H. T. Lee,S. C. Lee,C. Leluc,Giuseppe Levi,H. L. Li,J. Q. Li,Qiang Li,T. X. Li,Wei Li,Y. Li,Z. H. Li,Z. Y. Li,S. Lim,Chia-Hui Lin,P. Lipari,Thomas Lippert,Dong Liu,Hengchang Liu,M. Lolli,Teimuraz Lomtadze,M. J. Lu,S. Q. Lu,Ying Lu,K. Luebelsmeyer,J. Z. Luo,S. S. Lv,R. D. Majka,C. Mañá,J. C. Marin,Tim Martin,G. Martinez,N. Masi,David Maurin,A. Menchaca-Rocha,Q. Meng,D. C. Mo,Luca Morescalchi,P. Mott,M. Müller,J. Q. Ni,N. Nikonov,F. Nozzoli,P. Nunes,A. Obermeier,A. Oliva,M. Orcinha,F. Palmonari,C. Palomares,M. Paniccia,A. Papi,M. Pauluzzi,E. Pedreschi,S. Pensotti,R. Pereira,N. Picot-Clemente,Fabrizio Giulio Luca Pilo,A. Piluso,C. Pizzolotto,V. Plyaskin,M. Pohl,V. Poireau,E. Postaci,Antje Putze,Lucio Quadrani,X. M. Qi,Xubo Qin,Z. Y. Qu,T. Räihä,Pier-Giorgio Rancoita,D. Rapin,J. S. Ricol,I. Rodríguez,S. Rosier-Lees,A. Rozhkov,Davide Rozza,Roald Z. Sagdeev,J. Sandweiss,P. Saouter,C. Sbarra,S. Schael,S. M. Schmidt,A. Schulz von Dratzig,G. Schwering,G. Scolieri,Eun-Suk Seo,B. S. Shan,Y. H. Shan,J. Y. Shi,X. Y. Shi,Yun Shi,T. Siedenburg,Dong-Chul Son,F. Spada,F. Spinella,Won Kyu Calvin Sun,W. H. Sun,Mauro Tacconi,C. P. Tang,X. W. Tang,Zhixiang Tang,L. Tao,D. Tescaro,Samuel C.C. Ting,S. M. Ting,Nicola Tomassetti,J. J. Torsti,C. Türkoğlu,T. Urban,V. Vagelli,E. Valente,C. Vannini,Eino Valtonen,S. S. Vaurynovich,M. Vecchi,Mayda Velasco,J. P. Vialle,V. Vitale,S. Vitillo,Liqiu Wang,Naihua Wang,Q. L. Wang,Ruiguang Wang,Xiaoping Wang,Zheng Wang,Z. L. Weng,K. Whitman,J. Wienkenhöver,H. Wu,Xin Wu,X. Xia,M. Xie,S. Xie,R. Q. Xiong,Gongming Xin,Ningsheng Xu,W. Xu,Qing-Bo Yan,J. Yang,Mingming Yang,Q. H. Ye,H. Yi,Y. J. Yu,Z. Q. Yu,S. Zeissler,J. H. Zhang,M. T. Zhang,X. B. Zhang,Zhijun Zhang,Z. M. Zheng,H. L. Zhuang,Valery Zhukov,A. Zichichi,N. Zimmermann,Paolo Zuccon,C. Zurbach +294 more
TL;DR: In this paper, a precise measurement of the proton flux in primary cosmic rays with rigidity (momentum/charge) from 1.GV to 1.8TV is presented based on 300 million events.
High Statistics Measurement of the Positron Fraction in Primary Cosmic Rays of 0.5-500 GeV with the Alpha Magnetic Spectrometer on the International Space Station
L. Accardo,M. Aguilar,D. Aisa,D. Aisa,Behcet Alpat,A. Alvino,G. Ambrosi,K. Andeen,Luísa Arruda,N. Attig,Philipp Azzarello,Philipp Azzarello,A. Bachlechner,Fernando Barão,A. Barrau,L. Barrin,A. Bartoloni,L. Basara,Markus Battarbee,Roberto Battiston,J. Bazo,U. Becker,M. Behlmann,B. Beischer,J. Berdugo,B. Bertucci,B. Bertucci,G. Bigongiari,Veronica Bindi,S. Bizzaglia,M. Bizzarri,M. Bizzarri,G. Boella,W. De Boer,K. Bollweg,V. Bonnivard,B. Borgia,S. Borsini,Matteo Boschini,M. Bourquin,J. D. Burger,Franck Cadoux,X. D. Cai,M. Capell,S. Caroff,Gianpaolo Carosi,J. Casaus,V. Cascioli,G. Castellini,I. Cernuda,D. Cerreta,D. Cerreta,F. Cervelli,M. J. Chae,Y. H. Chang,A. I. Chen,H. S. Chen,G. M. Cheng,H. S. Chen,Lin Cheng,A. Chikanian,H. Y. Chou,E. Choumilov,V. Choutko,C. H. Chung,Federico Cindolo,C. Clark,R. Clavero,G. Coignet,C. Consolandi,A. Contin,Claudio Corti,B. Coste,Z. Cui,M. Dai,C. Delgado,S. Della Torre,M. B. Demirköz,Laurent Derome,S. Di Falco,L. Di Masso,L. Di Masso,F. Dimiccoli,Carlos Díaz,P. von Doetinchem,W. J. Du,M. Duranti,D. D'Urso,A. Eline,F. J. Eppling,T. Eronen,Y. Y. Fan,L. Farnesini,J. Feng,E. Fiandrini,E. Fiandrini,A. Fiasson,E. Finch,Peter H. Fisher,Yu. Galaktionov,G. Gallucci,Bruce Rafael Mellado Garcia,R. J. García-López,Henning Gast,I. Gebauer,Massimo Gervasi,A. Ghelfi,W. Gillard,F. Giovacchini,P. Goglov,J. Gong,C. Goy,Varlen Grabski,D. Grandi,M. Graziani,M. Graziani,C. Guandalini,I. Guerri,K. H. Guo,D. Haas,M. Habiby,Sadakazu Haino,Sadakazu Haino,K. C. Han,Z. H. He,Matthias Heil,Matthias Heil,R. Henning,J. Hoffman,Timothy H. Hsieh,Zhiqi Huang,Changgi Huh,M. Incagli,Maria Ionica,W. Y. Jang,H. Jinchi,K. Kanishev,G. N. Kim,Kwangsoo Kim,T. Kirn,R. Kossakowski,O. Kounina,Andrei Kounine,V. Koutsenko,M. S. Krafczyk,S. Kunz,G. La Vacca,E. Laudi,E. Laudi,G. Laurenti,I. Lazzizzera,A. Lebedev,H. T. Lee,S. C. Lee,C. Leluc,Giuseppe Levi,H. L. Li,J. Q. Li,Qiang Li,T. X. Li,Wei Li,Y. Li,Z. H. Li,Z. Y. Li,S. Lim,Chia-Hui Lin,P. Lipari,Thomas Lippert,Dong Liu,Hengchang Liu,M. Lolli,Teimuraz Lomtadze,M. J. Lu,Ying Lu,K. Luebelsmeyer,F. Luo,J. Z. Luo,S. S. Lv,R. D. Majka,A. Malinin,C. Mañá,J. C. Marin,Tim Martin,G. Martinez,N. Masi,F. Massera,David Maurin,Arturo Alejandro Menchaca-Rocha,Q. Meng,D. C. Mo,Benjamin Monreal,Luca Morescalchi,P. Mott,M. Müller,J. Q. Ni,N. Nikonov,F. Nozzoli,P. Nunes,A. Obermeier,A. Oliva,M. Orcinha,F. Palmonari,C. Palomares,M. Paniccia,A. Papi,M. Pauluzzi,M. Pauluzzi,E. Pedreschi,S. Pensotti,R. Pereira,R. Pilastrini,Fabrizio Giulio Luca Pilo,A. Piluso,A. Piluso,C. Pizzolotto,V. Plyaskin,M. Pohl,V. Poireau,E. Postaci,Antje Putze,Lucio Quadrani,X. M. Qi,P. G. Rancoita,D. Rapin,J. S. Ricol,I. Rodríguez,S. Rosier-Lees,Lucio Rossi,A. Rozhkov,Davide Rozza,G. Rybka,Roald Z. Sagdeev,J. Sandweiss,P. Saouter,C. Sbarra,S. Schael,S. M. Schmidt,D. Schuckardt,A. Schulz von Dratzig,G. Schwering,G. Scolieri,Eun-Suk Seo,B. S. Shan,Y. H. Shan,J. Y. Shi,X. Y. Shi,Yun Shi,T. Siedenburg,Dong-Chul Son,F. Spada,F. Spinella,Won Kyu Calvin Sun,W. H. Sun,Mauro Tacconi,C. P. Tang,X. W. Tang,Zhixiang Tang,L. Tao,D. Tescaro,Samuel C.C. Ting,S. M. Ting,Nicola Tomassetti,J. J. Torsti,C. Türkoʇlu,T. Urban,V. Vagelli,E. Valente,C. Vannini,Eino Valtonen,S. S. Vaurynovich,Manuela Vecchi,Mayda Velasco,J. P. Vialle,V. Vitale,G. Volpini,Liqiu Wang,Q. L. Wang,Ruiguang Wang,Xiaoping Wang,Zheng Wang,Z. L. Weng,K. Whitman,J. Wienkenhöver,H. Wu,K. Y. Wu,X. Xia,M. Xie,S. Xie,R. Q. Xiong,Gongming Xin,Ningsheng Xu,W. Xu,Q. Yan,J. Yang,Mingming Yang,Q. H. Ye,H. Yi,Y. J. Yu,Z. Q. Yu,S. Zeissler,J. H. Zhang,M. T. Zhang,X. B. Zhang,Zhijun Zhang,Z. M. Zheng,Fei Zhou,H. L. Zhuang,Valery Zhukov,Antonino Zichichi,N. Zimmermann,Paolo Zuccon,C. Zurbach +311 more
TL;DR: The new results show, for the first time, that above ∼200 GeV the positron fraction no longer exhibits an increase with energy.
Flaring-associated Complex Dynamics in Two M Dwarfs Revealed by Fast, Time-resolved Spectroscopy
J. Wang,H. L. Li,Li-Ping Xin,G. Li,Jie Bai,C. Gao,Bin Ren,Deheng Song,Jinsong Deng,Z. G. Dai,En-Wei Liang,X. Y. Wang,J. Y. Wei +12 more
TL;DR: In this article , the authors reported an observational study on the flares of two M dwarfs triggered by the high-cadence survey performed by the Ground-based Wide Angle Camera system, which revealed symmetric broad Hα emission with not only a nearly zero bulk velocity, but also a large projected maximum velocity as high as ∼700-800 km s−1.
11
[Fibrocartilaginous lipoma: a clinicopathological analysis of six cases].
H. L. Li,J Wang,H. Cheng,S. Zhang,Rong-jun Mao +4 more
- 08 Aug 2023
TL;DR: Fibrocartilaginous lipoma is a benign lipomatous tumor with mature adipocytes, fibrocartilage and fibrous elements that helps the distinction from its morphologic mimics.
Photometric Observations of Flares on AD Leo from GWAC-F30 and TESS
TL;DR: In this paper , the authors observed active M dwarf star AD Leo for 146 hours in photometry by GWAC-F30 and also analyzed 528 hr of photometric data of the star from the Transiting Exoplanet Survey Satellite (TESS).