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David R. Williams

3 papers hereh-index 14 citations2 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author2
  • last author1

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3
same name
  • David R. Williams — 19 papers, h 23
  • David R. Williams — 5 papers, h 28
  • David R. Williams — 2 papers
  • David R. Williams — 2 papers, h 5
  • David R. Williams — 1 paper, h 2

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20222025
most citedEvolution of the critical torus instability height and CME likelihood in solar active regions

13 citations · 14 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2025

Solar Orbiter's 2024 Major Flare Campaigns: An Overview

Daniel F. Ryan, Laura A. Hayes, Hannah Collier +17

Solar Orbiter conducted a series of flare-optimised observing campaigns in 2024 utilising the Major Flare Solar Orbiter Observing Plan (SOOP). Dedicated observations were performed…

astro-ph.SR2024★ 1 cited

How does the critical torus instability height vary with the solar cycle?

Alexander W. James, Lucie M. Green, Graham Barnes +2

The ideal magnetohydrodynamic torus instability can drive the eruption of coronal mass ejections. The critical threshold of magnetic field strength decay for the onset of the torus…

astro-ph.SR2022★ 13 cited

Evolution of the critical torus instability height and CME likelihood in solar active regions

Alexander W. James, David R. Williams, Jennifer O'Kane

Aims. Working towards improved space weather predictions, we aim to quantify how the critical height at which the torus instability drives coronal mass ejections (CMEs) varies over…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.