• Publications
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Three‐dimensional, multispecies, high spatial resolution MHD studies of the solar wind interaction with Mars
[1] We present the results of model calculations, using our new, four-species, spherical MHD model. Our results are compared with the relevant and limited available data. The resulting comparisonsExpand
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Space Weather Modeling Framework: A new tool for the space science community
[1] The Space Weather Modeling Framework (SWMF) provides a high-performance flexible framework for physics-based space weather simulations, as well as for various space physics applications. The SWMFExpand
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Adaptive numerical algorithms in space weather modeling
TLDR
Space weather describes the various processes in the Sun-Earth system that present danger to human health and technology. Expand
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Modeling a space weather event from the Sun to the Earth: CME generation and interplanetary propagation
[1] We present a three-dimensional (3-D) numerical ideal magnetohydrodynamics (MHD) model describing the time-dependent expulsion of a coronal mass ejection (CME) from the solar corona propagating toExpand
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A Three-dimensional Model of the Solar Wind Incorporating Solar Magnetogram Observations
We present a new compressible MHD model for simulating the three-dimensional structure of the solar wind under steady state conditions. The initial potential magnetic field is reconstructedExpand
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Relativistic laser piston model: Ponderomotive ion acceleration in dense plasmas using ultraintense laser pulses
Laser ponderomotive force at superhigh intensities provides an efficient ion acceleration in bulk dense targets and evacuates a channel enabling further laser beam propagation. The developedExpand
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CRASH: A BLOCK-ADAPTIVE-MESH CODE FOR RADIATIVE SHOCK HYDRODYNAMICS—IMPLEMENTATION AND VERIFICATION
TLDR
We describe the Center for Radiative Shock Hydrodynamics (CRASH) code, a block-adaptive-mesh code for multi-material radiation hydrodynamICS. Expand
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MAGNETOHYDRODYNAMIC WAVES AND CORONAL HEATING: UNIFYING EMPIRICAL AND MHD TURBULENCE MODELS
We present a new global model of the solar corona, including the low corona, the transition region, and the top of the chromosphere. The realistic three-dimensional magnetic field is simulated usingExpand
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Dynamics of emitting electrons in strong laser fields
A new derivation of the motion of a radiating electron is given, leading to a formulation that differs from the Lorentz–Abraham–Dirac equation and its published modifications. It satisfies the properExpand
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Understanding SDO/AIA Observations of the 2010 June 13 EUV Wave Event: Direct Insight from a Global Thermodynamic MHD Simulation
In this work, we present a comprehensive observation and modeling analysis of the 2010 June 13 extreme-ultraviolet (EUV) wave observed by the Atmospheric Imaging Assembly (AIA) aboard the SolarExpand
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