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D. Williams

3 papers hereh-index 2141 citations4 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-ph1
  • astro-ph.HE1
  • astro-ph.SR1
same name
  • D. Williams — 160 papers, h 50
  • D. Williams — 116 papers, h 0
  • D. Williams — 107 papers, h 29
  • D. Williams — 77 papers, h 19
  • D. Williams — 69 papers, h 73
  • D. Williams — 18 papers, h 17

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
20052026
most citedThe first observed stellar X-ray flare oscillation: Constraints on the flare loop length and the magnetic field

114 citations · 155 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2026

Probing Physical Conditions in Classical and Symbiotic Novae with the Square Kilometre Array Observatory

Rocco Lico, Marcello Giroletti, Arnau Aguasca-Cabot +9

Cataclysmic variables and symbiotic stars are interacting binary systems in which a hot white dwarf (WD) orbits a companion main-sequence or red giant star, respectively. Accumulat…

astro-ph.SR2013★ 41 cited

Measuring the Magnetic Field Strength of the Quiet Solar Corona Using "EIT Waves"

David M. Long, David R. Williams, Stéphane Régnier +1

Variations in the propagation of globally-propagating disturbances (commonly called "EIT waves") through the low solar corona offer a unique opportunity to probe the plasma paramet…

astro-ph2005★ 114 cited

The first observed stellar X-ray flare oscillation: Constraints on the flare loop length and the magnetic field

U. Mitra-Kraev, L. K. Harra, D. R. Williams +1

We present the first X-ray observation of an oscillation during a stellar flare. The flare occurred on the active M-type dwarf AT Mic and was observed with XMM-Newton. The soft X-r…

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