Physics
Scientist
University of Texas at Dallas, Richardson, TX, US
Center for Space Sciences, Univ of Texas at Dallas, Richardson, TX, USA ; Royal Institute of Technology, Space & Plasma Physics, Stockholm, Sweden and Plasma Physics, School of Electrical Engineering, Royal Institute of Technology
University of Texas at Dallas, Center for Space Sciences PO Box 830688, FO22, Richardson, TX 75083-0688, USA; Alfvén Laboratory, Royal Institute of Technology, School of Electrical Engineering, Stockholm, SE-100 44 Sweden
Alfvén Laboratory, Royal Institute of Technology, School of Electrical Engineering, Stockholm, SE-10044 Sweden; University of Texas at Dallas, Center for Space Sciences, PO Box 830688, FO22, Richardson, TX 75083, USA
Texas Univ. at Dallas, Richardson
Center for Space Sciences, University of Texas at Dallas, Richardson, Texas, USA
Alfvén Laboratory, Royal Institute of Technology, Stockholm SE-100 44, Sweden
Alfvén Laboratory, Royal Institute of Technology, Stockholm 100 44, Sweden; Center for Space Sciences, University of Texas at Dallas
Alfvén Laboratory, Royal Institute of Technology, 10044 Stockholm, Sweden
Center for Space Sciences, University of Texas at Dallas, Richardson, TX, USA; Alfvén Laboratory, Royal Institute of Technology, Stockholm, Sweden
University of Texas at Dallas, Center for Space Sciences POB 830688, FO22, Richardson, TX 75025, USA; Alfven Laboratory, Royal Institute of Technology, Stockholm, SE-100 44 Sweden
Alfvén Laboratory, Royal Institute of Technology, Stockholm, SE-10044, Sweden; William B. Hanson Center for Space Sciences, University of Texas at Dallas, Richardson, TX 75083, USA Center for Space Sciences, University of Texas at Dallas, Richardson, TX, USA
University of Texas at Dallas, Center for Space Sciences PO Box 830688 MS / FO22, Richardson, TX 75083-0688, USA; Alfven
Electric fields in the Hermean environment
Electromagnetic Phenomena in Mercury's Magnetosphere
Erratum: ``Ionospheric convection response to slow, strong variations in a northward interplanetary magnetic field: A case study for January 14, 1988'' [J. Geophys. Res., 98, 19,273-19,292 (1993)
Evolution in space and time of the quasi-static acceleration potential of inverted-V aurora and its interaction with Alfvénic boundary processes
Evolution of the global aurora during positive IMF <formula>Bz and varying IMF <formula>By conditions
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