Astronomy and Astrophysics – Astrophysics – Instrumentation and Methods for Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Instrumentation and Methods for Astrophysics
Scientist
University of Durham
National Solar Observatory, USA
University of Durham, United Kingdom
The Pennsylvania State University, USA
National Solar Observatory, Sunspot, NM 88349 Astronomical Observatoires / Nanjing Institute of Astronomical Optics and Technology, Chinese Academy of Sciences, Nanjing, China; Physics and Astronomy Department, California State University, Northridge, CA State University, Northridge, USA
National Astronomical Observatories / Nanjing Institute of Astronomical Optics & Technology, Chinese Academy of Sciences, Nanjing 210042, China; Key Laboratory of Astronomical Optics & Technology, Nanjing Institute of Astronomical Optics & Technology, Chinese Academy of Sciences, Nanjing 210042, China; Physics and Astronomy Department, California State University Northridge, 18111 Nordhoff Street, Northridge, CA 91330-8268 of Astronomy and Astrophysics, 525 Davey Laboratory, Penn State University, University Park, PA 16802 Instrumentation Group, University of Durham, Physics Department, South Road, Durham, DH1 3LE, UK; National Solar Observatory, P.O. Box 62, Sunspot, NM 88349 of Physics, New Jersey Institute of Technology, Newark, NJ 07102
New Jersey Institute of Technology, USA
Durham University, UK
National Solar Observatory, Sunspot, NM 88349 of Texas at Dallas / Geosciences, UTD Box 830688, Richardson, TX 75083-0688, USA University
New Jersey Institute of Technology, Center for Solar-Terrestrial Research, 323 Martin Luther King Blvd, Newark, NJ 07102-1982, USA; Big Bear Solar Observatory, 40386 North Shore Lane, Big Bear City, CA 92314-9672, USA
A Coronagraph Based on Stepped-Transmission Filters
A Coronagraph Using a Liquid Crystal Array and a Deformable Mirror for Active Apodizing and Phase Corrections
A portable solar adaptive optics system
A portable solar adaptive optics system: software and laboratory developments
A search for flaring very-high-energy cosmic γ-ray sources with the L3+C muon spectrometer
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