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Physics and Astronomy Department Rice University, MS-108, Houston, TX 77005-1892, USA
Rice University, Physics and Astronomy Department, MS 108, 6100 Main St, Houston, TX 77005-1892, USA
Department of Physics and Astronomy, Rice University, Houston, Texas, USA
Rice University, Houston, TX
Physics and Astronomy Department, Rice University, Houston, Texas, USA
Physics and Astronomy Department, MS 108, Rice University, Houston, TX 77005-1892, USA
Department of Physics and Astronomy, William Marsh Rice University, Houston, Texas, USA
Physics and Astronomy Department, Rice University, 6100 South Main St., Houston, TX 77005, USA
Department of Physics and Astronomy, Rice University, MS 108, P. O. Box 1892, Houston, TX 77251, USA
RIce University, Physics and Astronomy Dept, MS 108, 6100 Main St, Houston, TX 77005-1892, USA
Department of Physics and Astronomy, Rice University, MS-108 6100 Main St., Houston, TX 77005, USA
Rice University, Physics and Astronomy Dept., MS-108, 6100 Main St., Houston, TX 77005-1892, USA
Physics and Astronomy Dept., Rice University, 202 Herman Brown Hall, 6100 Main Street, Houston, TX 77005, USA
Rice Univ., Houston, TX, US
Rice University, MS 108, Physics and Astronomy Dept, 6100 Main st, Houston, TX 77251, USA
Department of Physics and Astronomy, Rice University, Houston, TX 77251-1892, USA
Rice University, Physics and Astronomy Dept., MS108 P.O. Box 1892, Houston, TX 77251-1892, USA
Rice University, Physics and Astronomy Department, 6100 S Main St., MS-108, Houston, TX 77005, USA
Rice University, Physics and Astronomy Department MS-108, 6100 Main St., Houston, TX 77005, USA
Rice University, Department of Physics and Astronomy MS108 6100 Main Street, Houston, TX 77005, USA
Department of Physics a
A flexible approach to modeling the storm time Region 2 and magnetopause currents
A nonsingular model of the open magnetosphere
A tangent subsolar merging line
Accelerated thinning of the near-Earth plasma sheet caused by a bubble-blob pair
Calculation of Synthetic Ground Magnetograms From Current Distributions Calculated by Large-Scale Magnetosphere-Ionosphere Coupling Codes
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