TW
Member Since 2007
Tori D. Wilder
Assistant Professor, University of Texas at Arlington
AGU Research
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Unravelling the link between turbulence, intermittency, and dissipation in the terrestrial magnetosheath
MULTISCALE DYNAMICS IN MAGNETIZED TURBULENCE II ORAL
spa-solar and heliospheric physics | 13 december 2024
Alexandros Chasapis, Yi Qi, NEHA PATHAK, Narges Ah...
Turbulence is an inherently multiscale phenomenon. It is characterized by cross-scale energy transfer, along with the formation of intermittent struct...
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The Time Evolution of Whistler Waves Associated with Magnetic Reconnection in the Dayside Magnetopause
MAGNETIC RECONNECTION: CONNECTING IDEAS FROM OBSERVATIONS, EXPERIMENTS, MODELS, AND THEORY III POSTER
spa-magnetospheric physics | 13 december 2024
Richard Lott, Victoria D. Wilder, Matthew R. Argal...
The association between magnetic reconnection in the dayside magnetopause and plasma waves is well-documented, having been confirmed by various space ...
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MHD Simulation of a Kelvin Helmholtz Instability Observation by MMS in June 2020 using MAGE Model
DOWN TO EARTH WITH SPACE WEATHER: MAGNETIC STORM–INDUCED GEOELECTRIC FIELDS, CURRENTS, AND IMPACTS I POSTER
geomagnetism, paleomagnetism and electromagnetism | 12 december 2024
Oshina Jagtap, Victoria D. Wilder, Kevin H. Pham, ...
The Kelvin-Helmholtz Instability (KHI) is thought to be an important mechanism whereby energy and momentum are coupled from the solar wind to the magn...
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An Investigation into Lion Roar Harmonics using in-situ data in Earth’s Magnetosheath
DAYSIDE MAGNETOSPHERE INTERACTIONS II ORAL
spa-magnetospheric physics | 11 december 2024
Hector Salinas, Victoria D. Wilder, Narges Ahmadi,...
Satellite observations and simulations of Earths magnetosheath demonstrated that ion cyclotron and mirror instabilities contribute to regulating the d...
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Ion Acceleration Efficiency in Turbulent Quasi-Parallel Shock Crossings
DAYSIDE MAGNETOSPHERE INTERACTIONS III POSTER
spa-magnetospheric physics | 11 december 2024
Anansa Keaton-Ashanti, Victoria D. Wilder, Alexand...
Turbulence in large scale plasma structures typically occurs either through magnetic reconnection, flow braking, or shock region energy transfer. In t...
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Identifying the Traveling Atmospheric Disturbance (TAD) - related Traveling Ionospheric Disturbances (TIDs) in the Storm Time Ionosphere with NASA GDC AETHER
MAGNETOSPHERE-IONOSPHERE-THERMOSPHERE COUPLING DURING DISTURBED TIMES I POSTER
spa-aeronomy | 11 december 2024
Lauren Christenson, Naomi Maruyama, Laila Andersso...
Geospace Dynamics Constellation (GDC) is an upcoming NASA mission that aims to understand the response of Earths upper atmosphere to magnetic storms. ...
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Parallel Electric Fields During Observations of the Earth’s Alfvén Wings
THREE-DIMENSIONAL MAGNETOSPHERE STRUCTURE AND DYNAMICS DURING GEOMAGNETIC STORMS II ORAL
spa-magnetospheric physics | 11 december 2024
Victoria D. Wilder, Li-Jen Chen, Brandon L. Burkho...
During nominal conditions, the solar wind is super-Alfvénic. Simulations and observations have shown that during prolonged periods when the solar wind...
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Global Magnetic Reconnection with Weakly Shocked Solar Wind During Geomagnetic Storms
THREE-DIMENSIONAL MAGNETOSPHERE STRUCTURE AND DYNAMICS DURING GEOMAGNETIC STORMS I POSTER
spa-magnetospheric physics | 11 december 2024
Brandon L. Burkholder, Li-Jen Chen, Victoria D. Wi...
The solar wind and magnetic field emanating from the sun typically reaches Earth moving at a super-Alfvenic velocity (multiple times the local Alfven ...
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