Nonlinear Sciences – Pattern Formation and Solitons
Scientist
Nonlinear Sciences
Pattern Formation and Solitons
Scientist
Uni. Frankfurt
Department of Physics and Center for Atmospheric and Space Science, Utah State University, Logan, Utah, USA
Polar Research Institute of China, 451 Jinqiao Road., Shanghai 200136, China
Yunnan Observatory of National Observatoires, Chinese Academy of Science, Yunnan Province 650011, China of Astronomy, Nanjing University, 22 Hankou Lu, Nanjing, Jiangsu 210093, China
Institute of Geology, CAGS, 26 Baiwanzhuang Rd., Beijing 100037, China
Center for Atmospheric and Space Science, Utah State University, CASS, Utah State University, Logan, UT 84322-4405, USA
Yunnan Astronomical Observatory, National Astronomical Observatoires, Kunming 650011, China
Chinese Academy of Sciences, Institute of Geochemistry, Guiyang, People's Republic of China
Chinese Academy of Science, Beijing, China
Laboratoire d'Études Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris, 5 Place Jules Janssen, F-92195 Meudon Cedex, France; and Astronomy Department, University of Nanjing, 210093 Nanjing, China
State Key Laboratory of High Field Laser Physics, Shanghai Institute of Optics and Fine Mechanics, Chinese Academy of Sciences, PO Box 800-211, Shanghai 201800, China
Utah State University, Center for Atmospheric and Space Sciences 4405 Old Main Hill, Logan, UT 84322-4405, USA of Physics and Center for Atmospheric and Space Science, Utah State University, Logan, UT, USA Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, PR China
Department of Astronomy, Nanjing University, Nanjing, 210093, China
Max-Planck-Institut für Sonnensystemforschung, Max-Planck-Strasse 2, 37191 Katlenburg-Lindau, Germany ; Yunnan Astronomical Observatory / National Astronomical Observatoires, Chinese Academy of Science, Kunming 650011, PR China Academy of Sciences, Institute of Geochemistry, Guiyang, People's Republic of China; Max-Planck-Institut für Chemie, Mainz, Germany
Astronomic
A criterion for testing multi-particle NPT entanglement
A multi-party correlation measure based on cumulant
A new radio spectral receiving system at lambda =13 MM in Urumqi Astronomical Station
A search for flaring very-high-energy cosmic γ-ray sources with the L3+C muon spectrometer
Advanced noise reduction techniques for ultra-low phase noise optical-to-microwave division with femtosecond fiber combs
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