HelioWebUniversity of California, San Diego, Department of Computer Science and Engineering
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Affiliated Works
sorted by decreasing year, and then by display-name
- An Accurate Structure of Alfven Soliton Formed by Modulational Interaction of the Lower Hybrid Waves With a Kinetic Alfven Mode
- Evidence for Compressive MHD Waves in the Solar Wind Near the Sun
- Hybrid simulations of solar wind interaction with magnetized asteroids: General characteristics of the interaction region
- Ion-Kinetic Tail Processes and Associated Ionospheric Signatures
- Radio Scattering Signature of High-Frequency Alfvén (Ion Cyclotron) Waves in the Inner Solar Wind
- Shock Surfing and Shock Drift Acceleration at a 2D Turbulent Front
- Time-dependent and Quasi-steady State Reconnection and Their Consequences at the Dayside Magnetopause
- Are Small Asteroids Magnetic?
- Characterization of Solar Wind Interaction With Magnetized Bodies
- Formation, Characteristics, and Diagnostic Usage of Energetic Ions in the Near and Mid Tail
- Solar Radar
- A New Method for Studying the Solar Wind Using Radio Scintillations (IPS)
- Component versus Anti-parallel Merging at the Magnetopause: Nonlinear Theory and Particle Simulations
- Hybrid and Hall MHD simulations of the out-of-the-plane magnetic field component: Origin and Generation Mechanism
- Ion Dynamics of the Inner Tail and Reconnection Signatures
- Ion-ion kink instability in the magnetotail: Linear Theory, Simulations and Comparison with Observations
- Linear Theory of Drift Tearing Modes at the Magnetopause
- Macrostructure of the Quasi-Parallel Shock and Magnetosheath: 1. Scale Lengths
- Macrostructure of the Quasi-Parallel Shock and Magnetosheath: 2. Nature of the ULF Waves
- Micrometeroid Flight in the Upper Atmosphere: Electron Emission and Charging
- Scaling of Magnetic Reconnection from Asteroids to Earth
- Stability and Structure of Superthin" Sheets: 2D and 3D Full Particle Simulations
- X-ray Emission From Planets Venus and Mars: Theoretical Model and Numerical Simulations
- 3D Seismogram Synthesis and Inversion for Finite Moment Tensors Using Receiver Green Tensors
- Alfvenic Turbulence Dissipation Near the Sun as Inferred From Radio Scattering Observations
- Bow Shock-Magnetosphere coupling under different IMF conditions
- Cyberinfrastructure for the Unified Study of Earth Structure and Earthquake Sources in Complex Geologic Environments
- Dusty Plasma Effects in Saturn's Rings
- Effect of different initialization methods on reconnection physics: A critical study using Hall MHD, hybrid, Hall-less hybrid and full particle simulations
- Formation of Plasmoids and Magnetic Flux Ropes during Southward IMF
- Global Hybrid Simulations of Solar Wind and Bow Shock Related Discontinuities Interacting with the Magnetosphere
- Ion-kinetic Mapping Between the Magnetotail and the Ionosphere
- On linear theory of anisotropy instabilities in a current sheet
- Parallel, time asynchronous modeling of plasmas: Overcoming the computational challenges in traditional (MHD, Hall MHD, Full Particle, Hybrid, Vlasov) codes
- Questioning common wisdom on issues of (i) cause of fast magnetic reconnection, (ii) origin and scale of quadrupole magnetic structure, and (iii) physical reality of Sweet-Parker regime
- Questioning common wisdom on magnetic reconnection on issues of (i) anti-parallel vs component merging, (ii) 3D effects, and (iii) role of lower-hybrid drift instability
- Role of Electron Temperature Anisotropy in the Onset of Magnetic Reconnection
- Global Hybrid Simulations: Discontinuities, Current Sheets, and Reconnection
- Non-driven Reconnection as a function of guide field strength
- On linear theory of ion anisotropy instabilities in a current sheet
- Progress and Future Directions in Computational Modeling of Geospace Plasmas
- An Efficient Implementation of a Local Binning Algorithm for Digital Elevation Model Generation of LiDAR/ALSM Dataset
- Core Field Generation Mechanisms in Flux Transfer Events
- Enhanced Access to High-Resolution LiDAR Topography through Cyberinfrastructure- Based Data Distribution and Processing
- Macroscopic Elongation of the Diffusion Region: Theoretical and Observational Consequences
- Simulation Study of 3D Collisionless Reconnection
- The Structure and Stability of the Diffusion Region in Collisionless Magnetic Reconnection
- Toward a Defensible Catalogue of Properties That Typify the Electron Diffusion Region of Collisionless Magnetic Reconnection
- Decision-Making Using Real-Time Observations for Environmental Sustainability; an integrated 802.11 sensor network
- Fully Kinetic 3D Simulations of Collisionless Reconnection in Large-Scale Pair Plasmas
- Nonlinear Energy Balance Model of Particle Acceleration by Parallel Shock Waves
- Is Magnetic Reconnection Different in the Magnetotail than at the Magnetopause?
- Three Dimensional Dynamics of Collisionless Magnetic Reconnection in Large-Scale Pair Plasmas
- Instability of the strahl electron distribution and a halo formation in the solar wind
- Rolling Deck to Repository (R2R): Technical Design - Experiences and Lessons (Invited)
- The Big Ten earthquake scenarios for Southern California
- heavy ion acceleration at shocks
- 3D fully kinetic simulations of magnetic reconnection in asymmetric, anti-parallel configuration
- Dynamics of transitional region of the solar wind turbulence with heliocentric distance
- Induced Nonlinear Scattering of Magnetospherically Reflecting Whistlers
- The strahl electrons as a source of electrostatic whistler waves in the solar wind turbulence
- Numerical model of 3D VLF LH/whistler nonlinear interactions in the topside ionosphere
- Theory of Space Dusty Plasma
- Heavy Ion Distribution Function in Magnetic Reconnection Diffusion Region
- OpenTopography: Addressing Big Data Challenges Using Cloud Computing, HPC, and Data Analytics
- Creation a Geo Big Data Outreach and Training Collaboratory for Wildfire Community
- Determining Methane Leak Locations and Rates with a Wireless Network Composed of Low-Cost, Printed Sensors
- How Much Can the Total Aleatory Variability of Empirical Ground Motion Prediction Equations Be Reduced Using Physics-Based Earthquake Simulations?
- Quantification of Ground Motion Reductions by Fault Zone Plasticity with 3D Spontaneous Rupture Simulations
- geoKepler Workflow Module for Computationally Scalable and Reproducible Geoprocessing and Modeling
- A community dataspace for distribution and processing of "long tail" high resolution topography data
- Dynamic Rupture Simulations with Plastic Yielding in Fault Damage Zone
- Verification and Validation of High-Frequency (f<SUB>max</SUB> = 5 Hz) Ground Motion Simulations of the 2014 M 5.1 La Habra, California, earthquake
- Eikonal tomography constrained by local sparse and low-rank matrix factorization
- Improving scientific data discovery and access - a case study using high resolution topography data in OpenTopography
- The SCEC Software Ecosystem for Earthquake System Science Research
- Web-based Topographic Differencing of High Resolution Topography Data
- A machine learning approach to data editing and rescue for global bathymetry models
- Beyond Search: Metadata Enhancement and In-Depth Data Exploration in EarthCube Data Discovery Studio.
- Factors Controlling the Release of Methylated Sulfur Species from Laboratory Mesocosm Experiments in Coastal Seawater
- New Advances in CyberShake PSHA Models
- On-Demand 3D topographic differencing hosted by OpenTopography
- Rapid Visualization and Analysis of ICESat-2 Data using an Intuitive GUI and JupyterHub Notebooks
- SeedMeLab: Search, manage, share and visualize data, like never before
- Building a spatially-explicit knowledge graph integrating health, pathogen and environmental data for COVID-19 analysis