PIC simulations of oblique shocks in turbulent plasma show that pre-existing 15% compressive turbulence produces a shorter hotter foreshock and more numerous higher-energy non-thermal electrons.
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3 Pith papers cite this work. Polarity classification is still indexing.
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Detection of helium lines in Balmer-dominated shocks of Type Ia SNRs reveals enhanced helium in some remnants and challenges shock models, enabling new constraints on progenitor environments.
Self-consistent 3D simulations from supernova explosion to remnant phase for six Type Ia models produce diverse X-ray spectra with asymmetric line profiles that match observed variations.
citing papers explorer
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PIC simulations of nonrelativistic high-Mach-number oblique shocks propagating in a turbulent medium
PIC simulations of oblique shocks in turbulent plasma show that pre-existing 15% compressive turbulence produces a shorter hotter foreshock and more numerous higher-energy non-thermal electrons.
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Helium emission from Balmer-dominated shocks in Type Ia supernova remnants provides constraints to their progenitor systems
Detection of helium lines in Balmer-dominated shocks of Type Ia SNRs reveals enhanced helium in some remnants and challenges shock models, enabling new constraints on progenitor environments.
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Probing the Diversity of Type Ia Supernova Remnants in 3-D Hydrodynamic Simulations with X-ray Spectral Synthesis
Self-consistent 3D simulations from supernova explosion to remnant phase for six Type Ia models produce diverse X-ray spectra with asymmetric line profiles that match observed variations.