University of Kansas, Department of Physics and Astronomy
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Affiliated Works
sorted by decreasing year, and then by display-name
- Heliospheric X-Rays and the 1/4 keV Soft X-Ray Background Map
- Modeling Titan's Upper Atmosphere with 1-D and 3-D Models:
- Saturn's A-ring Ionosphere as Observed by the Cassini Ion and Neutral Mass Spectrometer
- The Solar Wind Interaction With Mars and its Implications for Atmospheric Loss
- X-Ray Emission from the Terrestrial Magnetosheath
- Cassini-Huygens Ion Neutral Mass Spectrometer: Early Saturn and Titan Results
- Electron energetics of Titan's ionosphere
- Magnetospheric Electrons as a Source of Titan's Ionosphere: Model Comparisons with Cassini Data
- 3D Global MHD Simulation of Titan's interaction with its surrounding plasma
- Composition of Titan's ionosphere: A comparison of Cassini CAPS and INMS results
- Models of Thermal and Superthermal Electrons in Titan's Ionosphere
- Saturn Magnetospheric Interaction with Titan Ionisation Sources and Dynamics as Inferred from Cassini Observations
- Sensitivity of Titan's ENA emissions to incident ion flux and exospheric density
- Solar Radiation and Magnetospheric Electron Sources of the Ionosphere of Titan: Model Comparisons With Cassini Data
- Titan's Complex Neutral Composition as Measured by Cassini INMS
- Energetic Ion Precipitation at Titan
- Models of Titan's Ionosphere
- Quantifying the Exospheric Component of Soft X-ray Emission
- Spokes in Saturn's B Ring: Could Lightning be the Cause?
- The Precipitation of Energetic ions into Titan's Atmosphere
- Auroral X-ray Emission at Jupiter
- Observations of photoelectrons with CAPS ELS at Titan
- Properties of high-energy electrons at dawnside magnetosheath: Cassini observations during the earth swing-by 1999
- The Heliospheric Contribution to the Soft X-ray Background Emission
- The Plume Ionosphere of Enceladus as Seen by the Cassini Ion and Neutral Mass Spectrometer
- The Sheath Transport Observer for the Redistribution of Mass (STORM) Imager
- Titan's Plasma Interaction: New Perspectives from the Cassini Flybys
- Cometary airbursts and atmospheric chemistry: Tunguska and a candidate Younger Dryas event
- Dynamical and Magnetic Field Time Constants for Titan’s Ionosphere - Empirical Estimates
- Enceladus's Plumes: A Rocket Analogy
- Ion Loss from Titan's Atmosphere versus Local Time: A two-fluid MHD Study
- The Plasma Environments of Venus, Mars, and Titan: Implications for Atmospheric Escape (Invited)
- Electron Flux Modeling in the Enceladus Plume
- Hybrid Model Simulations Of Titan's Plasma Interactions
- Modeling the terrestrial radiation dose on planetary surfaces: A constraint on the habitability of Earth-like terrestrial planets
- Models of Electron Energetics in the Enceladus Torus
- Multi-fluid MHD study of Ion Loss from Titan's Atmosphere
- Ions in the Plume of Enceladus and the Role of Grain Interactions
- Multi-fluid MHD study of Titan's plasma interaction
- The Composition of Titan's Ionospheric Outflow
- Escape of Hot Oxygen Atoms from the Atmosphere of Mars
- Ions in the Plume of Enceladus and the Role of Grain Interactions
- On Lunar Exospheric Column Densities and Solar Wind Access Beyond the Terminator from ROSAT Soft X-ray Observations of Solar Wind Charge Exchange (SWCX)
- Dust Detection Using Radio and Plasma Wave Instruments in the Solar System
- Pickup Ions in the Plasma Environments of Mars, Comets, and Enceladus
- Solar Ionizing Radiation at Mars: Predictions vs. MAVEN Observations
- MAVEN Insights into the Precipitation of Solar Energetic Electrons in the Upper Atmosphere of Mars during the September 2017 ICME Event
- Magnetic Reconnection in the Collisional Ionosphere of Mars
- Modeling Ionospheric Densities and Flows in Crustal and Draped Magnetic Fields at Mars
- Saturn's Ionosphere in Light of Cassini Measurements
- Space Physics for a Small Program: What topics need to be covered?
- Alteration of crustal magnetic fields at Mars by currents induced by the solar wind interaction
- MHD momentum balance in the induced magnetic field at Mars using MAVEN data.
- Magnetic Fields, Atmospheres, and the Connection to Habitability (MACH) - Using Team Science to Determine How Magnetic Fields Influence Habitability
- Magnetic Reconnection in the Ionosphere of Mars: The Role of Collisions