activity
20162026
most citedEvolution of Cataclysmic Variables and Related Binaries Containing a White-Dwarf

79 citations · 197 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.SR2026

Multi-Height Spectropolarimetric Signatures of Magnetoacoustic Waves in Solar Plage

Taylor Sitterson, João M. da Silva Santos, Joshua Bentley +5

We analyze high-cadence spectropolarimetric observations of solar plage obtained with the Visible Spectro-Polarimeter (ViSP) on the Daniel K. Inouye Solar Telescope (DKIST) to inve…

astro-ph.SR2025

Ubiquitous high-frequency waves and disturbances in the active region corona observed with DKIST/Cryo-NIRSP

Momchil E. Molnar, Richard Morton, Alin Paraschiv +4

The plasma of the solar corona harbors a multitude of coronal wave modes, some of which could be dissipated to provide the required energy and momentum to heat the corona and accel…

astro-ph.SR2025

High-frequency coronal Alfvénic waves observed with DKIST/Cryo-NIRSP

Richard J. Morton, Momchil Molnar, Steven R. Cranmer +1

The presence and nature of low-frequency (0.1-10~mHz) Alfvénic waves in the corona has been established over the last decade, with many of these results coming from coronagraphic o…

astro-ph.SR2023

Magnetohydrodynamic Mode Conversion in the Solar Corona: Insights from Fresnel-like Models of Waves at Sharp Interfaces

Steven R. Cranmer, Momchil E. Molnar

The solar atmosphere is known to contain many different types of wavelike oscillation. Waves and other fluctuations (e.g., turbulent eddies) are believed to be responsible for at l…

astro-ph.SR2023★ 10 cited

Constraining the systematics of (acoustic) wave heating estimates in the solar chromosphere

Momchil E. Molnar, Kevin P. Reardon, Steven R. Cranmer +2

Acoustic wave heating is believed to contribute significantly to the missing energy input required to maintain the solar chromosphere in its observed state. We studied the propagat…

astro-ph.SR2023

Spatio-Temporal Comparisons of the Hydrogen-Alpha Line Width and ALMA 3 mm Brightness Temperature in the Weak Solar Network

Lucas A. Tarr, Adam R. Kobelski, Sarah A. Jaeggli +3

The strongest known correspondence between ALMA 3mm emission and other solar observations is between the H-alpha line width and 3 mm brightness temperature, while the typical 3-5mi…