activity
20112019
most citedObservation and Simulation of Longitudinal Oscillations of an Active Region Prominence

99 citations · 165 across the 6 of their papers we have counts for

collaborators

6 papers

math.AP2019★ 4 cited

Inviscid Limit for the Free-Boundary problems of MHD Equations with or without Surface Tension

Pengfei Chen, Shijin Ding

In this paper, we investigate the convergence rates of inviscid limits for the free-boundary problems of the incompressible magnetohydrodynamics (MHD) with or without surface tensi…

astro-ph.CO2017★ 11 cited

Fully Coupled Simulation of Cosmic Reionization. III. Stochastic Early Reionization by the Smallest Galaxies

Michael L Norman, Pengfei Chen, John H Wise +1

Previously we identified a new class of early galaxy that we estimate contributes up to 30\% of the ionizing photons responsible for reionization. These are low mass halos in the r…

math.AP2016★ 2 cited

Vanishing Viscosity Limit For the 3D Nonhomogeneous Incompressible Navier-Stokes Equations With a Slip Boundary Condition

Pengfei Chen, Yuelong Xiao, Hui Zhang

In this paper, we investigate the vanishing viscosity limit for the 3D nonhomogeneous incompressible Navier-Stokes equations with a slip boundary condition. We establish the local…

astro-ph.GA2014★ 39 cited

Scaling Relations for Galaxies Prior to Reionization

Pengfei Chen, John H. Wise, Michael L. Norman +2

The first galaxies in the Universe are the building blocks of all observed galaxies. We present scaling relations for galaxies forming at redshifts when reionization is…

astro-ph.SR2012★ 99 cited

Observation and Simulation of Longitudinal Oscillations of an Active Region Prominence

Qingmin Zhang, Pengfei Chen, Chun Xia +1

Filament longitudinal oscillations have been observed on the solar disk in H. We intend to find an example of the longitudinal oscillations of a prominence, where the magnetic d…

astro-ph.SR2011★ 10 cited

Where do flare ribbons stop?

P. F. Chen, J. T. Su, Y. Guo +1

The standard flare model, which was proposed based on observations and magnetohydrodynamic theory, can successfully explain many observational features of solar flares. However, th…