Physics
Scientist
Southwest Research Institute, San Antonio, Texas, USA
Southwest Research Institute, 6220 Culebra Rd., San Antonio, TX 78228, USA
Southwest Research Institute, 6220 Culdebra Road, San Antonio, TX 78228-0510, USA
Southwest Research Institute, Division of Space Science and Engineering, 6220 Culebra Road, San Antonio, TX 28510, USA
Southwest Research Institute, P.O. Drawer 28510, San Antonio, TX 78228-0510, USA Research Institute, Division of Space Science and Engineering, 6220 Culebra Road, San Antonio, TX 78228-0510, USA
Southwest Research Institute, 6220 Culebra Rd., San Antonio, TX 78228, USA Science and Engineering Division, Southwest Research Institute, San Antonio, Texas, USA
SwRI
Southwest Research Institute, Division of Space Science and Engineering, 6220 Culebra Road, San Antonio, TX 59812, USA Research Institute, 6220 Culebra Rd, San Antonio, TX 78228, USA
Southwest Research Institute, 9503 W Commerce, San Antonio, TX 78227, USA
Southwest Research Institute, PO Drawer 28510 Division 15, BLDG. 178, San Antionio, TX 78228-0510, USA
Goddard Space Flight Center
Southwest Research Institute, San Antonio, TX 78228-0510, USA
University of Michigan
Southwest Research Institute, Culebra Road, San Antonio, TX 78238, USA
Southwest Research Institute, 6220 Culebra Road, San Antonio, TX 78238, USA
Southwest Research Institute, San Antonio Res. Inst., San Antonio, TX, USA
Southwest Research Institute, Division of Space Science and Engineering, 9503 W Commerce, San Antonio, TX 78227-1, USA Research Institute, Post Office Box 28510, San Antonio, TX 78227-1, USA
Southwest Research Institute, P.O. Drawer 28510, San Antonio, TX 78228-0510,
3D Global MHD Simulation of Titan's interaction with its surrounding plasma
3D Multi-fluid Simulations With Ion-Neutral Interactions: Combining Observations and Modeling to Study Enceladus' Plume
A Multi-fluid Model of Enceladus: Plume Interactions With Saturn's Local Magnetospheric Flow
Advantages of Using a Multi-fluid Framework for Incorporating Ion-Neutral Interactions: Studying Enceladus` Interaction With Saturn`s Magnetosphere
Analysis of bow shock transition parameters at Jupiter from 140 to 1000 RJ
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