University of Texas, Arlington, Department of Physics

    flowchart
    I[University of Texas, Arlington, Department of Physics]
    PI["Parent Institutions (1)"]
    CI["Child Institutions (0)"]
    AW["Affiliated Works (58)"]
    CA["Linked Collaborating Authors (0)"]
    I== skos:broader ==>PI
    CI== skos:broader ==>I
    AW== affil ==>I
    AW== author ==>CA
    click PI "#parent-institutions"
    click CI "#child-institutions"
    click AW "#affiliated-works"
    click CA "#collaborating-authors"

ADS ID [?]

A11133

Abbreviation [?]

Dep Phy

Parent Institutions [?]

• University of Texas, Arlington

Child Institutions [?]

Affiliated Works

sorted by decreasing year, and then by display-name

• Generation Mechanism of S-Bursts at Jupiter and Earth: Initial Simulation Result
• DyFK Simulation of the O+ Density Trough at 5000 km Altitude in the Polar Cap
• DyFK-simulation-based formulaic representation of the effects of wave-driven ion heating and electron precipitation on ionospheric outflows
• Electron Acceleration on Jupiter-Io Flux Tube: Possible Generation Mechanism of S- Bursts
• O+ transport across the polar cap
• Wave Particle Diffusion of Energetic Ring Current Ions
• Alfvenic Acceleration of Io Torus Electrons
• Characteristics of low energy ions observed by New Horizon/SWAP during Jupiter's mangetotail flyby
• Determining the Viscous Potential from MHD Simulations and Comparing it to Observations
• Fluid-kinetic simulations of the passage of Storm Enhanced Density (SED) plasma flux tubes through the dayside cleft auroral processes region
• Magnetospheric Energy Coupling During CIR-Driven Storms
• Measures of Geo-effectiveness in Storms
• Physics-based formula representations of high-latitude ionospheric outflows: H+ and O+ densities and flow velocities vs. precipitation, wave-heating, and solar zenith angle effects
• Simulations of the formation of O+ trough zones in the polar cap ionosphere-magnetosphere coupling region
• Skill Scores for Ionospheric Modeling
• Studies of Magnetotail Dynamics and Energy Evolution During Substorms Using MHD Simulations
• The Current-Driven Magnetosphere
• The Use of Color as a Third Dimension on Maps
• Alfven Waves and Electron Energization and Their Interaction with Auroral Ionospheric Plasma Transport
• Comparison Between Data-Based and Simulation-Based Ion Outflow Scaling Laws
• Dynamic Fluid-Kinetic (DyFK) Simulations of Storm-Enhanced Density Supply of Cleft Ion Fountain Outflows
• Effect of Field-Aligned Potentials on Magnetospheric Dynamics at Jupiter and Saturn
• Effects of Solar Wind Parameters on the Energization of the Ring Current
• Generation of Parallel Electric Fields in the Jupiter-Io Torus Wake Region
• High-latitude ionospheric outflows characterized through analytic formulas
• Quasi-Stable Storm Reconnection Region
• Bow shock current closure for large IMF By: The unipolar generator
• Dual Reversed Convection and Magnetospheric Reconfiguration Under Strongly Northward IMF Conditions (Invited)
• On the Usefulness and Limitations of Empirical Ion Outflow Scaling Laws
• Primary heating mechanisms for the substantial neutral density enhancement in the cusp region
• SIMULATION OF TRANSPOLAR POTENTIAL SATURATION FOR NORTHWARD IMF
• Simulating the viscous interaction under a variety of solar wind conditions, with some comparisons to satellite data
• The Impact of Stereo Display on Student Understanding of Phases of the Moon
• The Lack of Ring Current Response to Large Y-Component IMF
• Contribution of Joule heating and soft particle precipitation to the cusp neutral density enhancement
• Factors that Affect Geoeffective Length for Northward IMF
• Sensitivity of magnetospheric energy input into the upper atmosphere from different models to the solar wind speed
• Comparison of LFM Simulation Results with Observation for Strongly Northward IMF
• Data and Model Views of Energy Input to the Dayside Thermosphere When the East-West Interplanetary Magnetic Field Is Large
• Estimates of the Geoeffective Length During the Whole Heliospheric Interval from Simulations
• Evolution of the Birkeland Currents During the Whole Heliosphere Interval from Various Simulations
• Geomagnetic energy variation during last solar cycle and its influence on the upper atmosphere
• Height Distribution of Joule Heating and its Influence on the Temperature and Density of the Upper Atmosphere
• Significance of Poynting flux and soft particle precipitation to the cusp neutral density enhancement
• Studying the Viscous Interaction during the Whole Heliosphere Interval
• Comparing the Viscous Potential from Virtual Satellite Passes Through the Low-Latitude Boundary Layer to Ionospheric Values, in an MHD Simulation
• Evidence of Decrease in Viscous Interaction during Events with Northward IMF as Seen in Lfm Simulation
• Height-Integrated Pedersen Conductivity in both E and F regions from COSMIC Observations
• Influence of non-hydrostatic processes on gravity-wave simulation in the upper atmosphere
• Penetration of IMF By into the Magnetotail in a Global MHD Simulation
• Wavelength dependence of solar flare irradiance enhancement and its influence on the thermosphere-ionosphere system
• Thermospheric winds around the cusp region
• A study of the non-linear response of the upper atmosphere to episodic and stochastic acoustic-gravity wave forcing
• Energy inputs in the polar cap during geomagnetic storms and the impacts on the ionosphere/thermosphere
• Inter-hemispheric asymmetry of Pedersen conductance
• Poynting flux distribution in the dayside polar cap boundary regions
• Grain Boundary Sliding in High Temperature Deformation of Directionally Solidified hcp Zn Alloys, and Implications for the Deformation Mechanism of Earth's Inner Core
• Can Interhemispheric Asymmetries in Ionospheric Outflow Wag the Magnetotail?

Linked Collaborating Authors [?]