237 citations · 1.2k across the 38 of their papers we have counts for
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Particle-in-cell simulations of particle energization via shock drift acceleration from low Mach number quasi-perpendicular shocks in solar flares
Jaehong Park, Chuang Ren, Jared C. Workman +1
Low Mach number, high beta fast mode shocks can occur in the magnetic reconnection outflows of solar flares. These shocks, which occur above flare loop tops, may provide the electr…
From Bipolar to Elliptical: Morphological Changes in the Temporal Evolution of PN
Martin Huarte Espinosa, Adam Frank, Bruce Balick +4
Proto-planetary nebulae (pPN) and planetary nebulae (PN) seem to be formed by interacting winds from asymptotic giant branch (AGB) stars. The observational issue that most pPN are…
Quantifying the Imprecision of Accretion Theory and Implications for Multi-Epoch Observations of Protoplanetary Discs
Eric G. Blackman, Farrukh Nauman, Richard G. Edgar
If accretion disc emission results from turbulent dissipation, then axisymmetric accretion theory must be used as a mean field theory: turbulent flows are at most axisymmetric only…