activity
20182025
most citedElement Abundances: A New Diagnostic for the Solar Wind

103 citations · 340 across the 8 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2025

Systematic non-thermal velocity increase preceding soft X-ray flare onset: A large-scale Hinode/EIS study

Andy S. H. To, Abigail Burden, Deborah Baker +12

Non-thermal velocities, derived from spectral line broadening, can provide crucial insights into plasma dynamics before and during solar flares. To systematically study the pre-fla…

astro-ph.SR2025

Estimating the Poynting flux of Alfvénic waves in polar coronal holes across Solar Cycle 24

Richard J. Morton, Micah J. Weberg, N. Balodhi +1

Alfvénic waves are known to be prevalent throughout the corona and solar wind. Determining the Poynting flux supplied by the waves is required for constraining their role in plasma…

astro-ph.SR2024

Assessing the Performance of the ADAPT and AFT Flux Transport Models Using In-Situ Measurements From Multiple Satellites

Kalman J. Knizhnik, Micah J. Weberg, Elena Provornikova +7

The launches of Parker Solar Probe (Parker) and Solar Orbiter (SolO) are enabling a new era of solar wind studies that track the solar wind from its origin at the photosphere, thro…

astro-ph.SR2023

Hinode EIS: updated in-flight radiometric calibration

G. Del Zanna, M. Weberg, H. P. Warren

We present an update to the in-flight radiometric calibration of the Hinode EUV Imaging Spectrometer (EIS), revising and extending our previous studies. We analyze full-spectral EI…

astro-ph.SR2019★ 103 cited

Element Abundances: A New Diagnostic for the Solar Wind

J. Martin Laming, Angelos Vourlidas, Clarence Korendyke +11

We examine the different element abundances exhibited by the closed loop solar corona and the slow speed solar wind. Both are subject to the First Ionization Potential (FIP) Effect…

astro-ph.SR2019★ 100 cited

A basal contribution from p-modes to the Alfvénic wave flux in the Sun's corona

R. J. Morton, M. Weberg, J. A. McLaughlin

Many cool stars possess complex magnetic fields [1] that are considered to undertake a central role in the structuring and energising of their atmospheres [2]. Alfvénic waves are t…