activity
20052023
most citedIonisation state, excited populations and emission of impurities in dynamic finite density plasmas. I: The generalised collisional-radiative model for light elements

264 citations · 3k across the 66 of their papers we have counts for

collaborators

66 papers

astro-ph.SR2023

The eruption of a magnetic flux rope observed by \textit{Solar Orbiter} and \textit{Parker Solar Probe}

David M. Long, Lucie M. Green, Francesco Pecora +11

Magnetic flux ropes are a key component of coronal mass ejections, forming the core of these eruptive phenomena. However, determining whether a flux rope is present prior to erupti…

astro-ph.SR2023★ 17 cited

A multiple spacecraft detection of the 2 April 2022 M-class flare and filament eruption during the first close Solar Orbiter perihelion

M. Janvier, S. Mzerguat, P. R. Young +56

The Solar Orbiter mission completed its first remote-sensing observation windows in the spring of 2022. On 2/4/2022, an M-class flare followed by a filament eruption was seen both…

astro-ph.SR2023★ 11 cited

Slow Solar Wind Connection Science during Solar Orbiter's First Close Perihelion Passage

Stephanie L. Yardley, Christopher J. Owen, David M. Long +76

The Slow Solar Wind Connection Solar Orbiter Observing Plan (Slow Wind SOOP) was developed to utilise the extensive suite of remote sensing and in situ instruments on board the ESA…

astro-ph.SR2023★ 17 cited

Understanding the Relationship between Solar Coronal Abundances and F10.7 cm Radio Emission

Andy S. H. To, Alexander W. James, T. S. Bastian +7

Sun-as-a-star coronal plasma composition, derived from full-Sun spectra, and the F10.7 radio flux (2.8 GHz) have been shown to be highly correlated (r = 0.88) during solar cycle 24…

astro-ph.SR2023

On orbit performance of the solar flare trigger for the Hinode EUV Imaging Spectrometer

David H. Brooks, Jeffrey W. Reep, Ignacio Ugarte-Urra +1

We assess the on-orbit performance of the flare event trigger for the Hinode EUV Imaging Spectrometer. Our goal is to understand the time-delay between the occurrence of a flare, a…

astro-ph.SR2023★ 27 cited

Observational Evidence of S-Web Source of the Slow Solar Wind

D. Baker, P. Demoulin, S. L. Yardley +25

From 2022 March 18-21, active region (AR) 12967 was tracked simultaneously by Solar Orbiter (SO) at 0.35 au and Hinode/EIS at Earth. During this period, strong blue-shifted plasma…