activity
20092022
most citedArborZ: Photometric Redshifts Using Boosted Decision Trees

128 citations · 303 across the 7 of their papers we have counts for

collaborators

7 papers

physics.plasm-ph2022★ 10 cited

Exploring the parameter space of MagLIF implosions using similarity scaling. III. Rise-time scaling

D. E. Ruiz, P. F. Schmit, M. R. Weis +2

Magnetized Liner Inertial Fusion (MagLIF) is a z-pinch magneto-inertial-fusion (MIF) concept studied on the Z Machine at Sandia National Laboratories. Two important metrics charact…

physics.plasm-ph2022★ 39 cited

Exploring the parameter space of MagLIF implosions using similarity scaling. II. Current scaling

D. E. Ruiz, P. F. Schmit, D. A. Yager-Elorriaga +9

Magnetized Liner Inertial Fusion (MagLIF) is a magneto-inertial-fusion (MIF) concept, which is presently being studied on the Z Pulsed Power Facility. The MagLIF platform has achie…

physics.plasm-ph2020★ 17 cited

Quantification of MagLIF morphology using the Mallat Scattering Transformation

Michael E. Glinsky, Thomas W. Moore, William E. Lewis +7

The morphology of the stagnated plasma resulting from Magnetized Liner Inertial Fusion (MagLIF) is measured by imaging the self-emission x-rays coming from the multi-keV plasma. Eq…

astro-ph.GA2020★ 78 cited

From parallel to perpendicular -- On the orientation of magnetic fields in molecular clouds

D. Seifried, S. Walch, M. Weis +4

We present synthetic dust polarization maps of simulated molecular clouds (MCs) with the goal to systematically explore the origin of the relative orientation of the magnetic field…

physics.comp-ph2019

Quantification of MagLIF morphology using the Mallat Scattering Transformation

Michael E. Glinsky, Thomas W. Moore, William E. Lewis +7

The morphology of the stagnated plasma resulting from Magnetized Liner Inertial Fusion (MagLIF) is measured by imaging the self-emission x-rays coming from the multi-keV plasma, an…

astro-ph.GA2018★ 31 cited

On the resolution requirements for modelling molecular gas formation in solar neighbourhood conditions

P. R. Joshi, S. Walch, D. Seifried +3

The formation of molecular hydrogen (H) and carbon monoxide (CO) is sensitive to the volume and column density distribution of the turbulent interstellar medium. In this paper,…