142 citations · 717 across the 22 of their papers we have counts for
22 papers
Direct calculation of steady-state hydrodynamic solar wind solutions with newtonian viscosity
Roger B. Scott, Stephen J. Bradshaw, Mark G. Linton +2
Steady-state solutions to the Navier-Stokes equations are known to admit solutions that are singular at the sonic point. Consequently, inviscid solar wind models require special tr…
Simulation of Thermal Nonequilibrium Cycles in the Solar Wind
Roger B. Scott, Jeffrey W. Reep, Mark G. Linton +1
Thermal nonequilibrium (TNE) is a condition of the plasma in the solar corona in which the local rate of energy loss due to radiation increases to the point that it cannot be susta…
Wave Steepening and Shock Formation in Ultracold Neutral Plasmas
M. K. Warrens, N. P. Inman, G. M. Gorman +3
We present observations of wave steepening and signatures of shock formation during expansion of ultracold neutral plasmas formed with an initial density distribution that is centr…
Modeling Realistic Heating Profiles of Transition Region Hot Loops on the Sun: Evidence for Impulsive Heating and Non-equilibrium Ionization
Shah Mohammad Bahauddin, Stephen J Bradshaw
The study examines the heating profile of hot solar transition region loops, particularly focusing on transient brightenings observed in IRIS 1400Å slit-jaw images. The findings ch…
Determining the nanoflare heating frequency of an X-ray Bright Point observed by MaGIXS
Biswajit Mondal, P. S. Athiray, Amy R. Winebarger +18
Nanoflares are thought to be one of the prime candidates that can heat the solar corona to its multi-million kelvin temperature. Individual nanoflares are difficult to detect with…
Magnetic Energy Powers the Corona: How We Can Understand its 3D Storage & Release
Amir Caspi, Daniel B. Seaton, Roberto Casini +12
The coronal magnetic field is the prime driver behind many as-yet unsolved mysteries: solar eruptions, coronal heating, and the solar wind, to name a few. It is, however, still poo…