activity
20062023
most citedThe solar chromosphere at high resolution with IBIS. I. New insights from the Ca II 854.2 nm line

147 citations · 1.3k across the 29 of their papers we have counts for

collaborators

29 papers

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…

astro-ph.IM2022

Helio2024 Science White Paper: ngGONG -- Future Ground-based Facilities for Research in Heliophysics and Space Weather Operational Forecast

Alexei A. Pevtsov, V. Martinez-Pillet, H. Gilbert +12

Long-term synoptic observations of the Sun are critical for advancing our understanding of Sun as an astrophysical object, understanding the solar irradiance and its role in solar-…

astro-ph.SR2022★ 56 cited

Defining the Middle Corona

Matthew J. West, Daniel B. Seaton, David B. Wexler +31

The middle corona, the region roughly spanning heliocentric altitudes from to , encompasses almost all of the influential physical transitions and processes that…

astro-ph.SR2022★ 6 cited

A spectroscopic survey of infrared 1-4μm spectra in regions of prominent solar coronal emission lines of Fe XIII, Si X, and Si IX

Aatiya Ali, Alin Paraschiv, Kevin Reardon +1

The infrared solar spectrum contains a wealth of physical data about the Sun and is being explored using modern detectors and technology with new ground-based solar telescopes. One…

astro-ph.SR2021★ 15 cited

A study of sunspot 3 minute oscillations using ALMA and GST

Yi Chai, Dale E. Gary, Kevin P. Reardon +1

Waves and oscillations are important solar phenomena, not only because they can propagate and dissipate energy in the chromosphere, but also because they carry information about th…