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W. Daughton

50 papers hereh-index 5710.6k citations406 works total

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

author position
  • first author1
  • middle author41
  • last author6

Across the 48 of 50 papers where every author was matched, so the position is known.

fields
  • physics.plasm-ph33
  • astro-ph.HE11
  • astro-ph.IM2
  • astro-ph.SR2
  • physics.space-ph2
same name
  • W. Daughton — 5 papers, h 8
  • W. Daughton — 1 paper

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
20092026
most citedFormation of Hard Power-laws in the Energetic Particle Spectra Resulting from Relativistic Magnetic Reconnection

461 citations · 2.3k across the 49 of their papers we have counts for

collaborators
Showing 2020 · physics.plasm-phShow all

3 papers · 2 filters

physics.plasm-ph2020

Mode Converting Alfvén Waves from Magnetic Reconnection Enhancing the Energy Source for the Aurora Borealis

Harsha Gurram, Jan Egedal, William Daughton

Previous studies have concluded that the Hall magnetic field structures generated during magnetic reconnection are carried away by kinetic Alfvén waves (KAW). Here we apply a kinet…

physics.plasm-ph2020★ 5 cited

Major Scientific Challenges and Opportunities in Understanding Magnetic Reconnection and Related Explosive Phenomena throughout the Universe

H. Ji, A. Alt, S. Antiochos +97

This white paper summarizes major scientific challenges and opportunities in understanding magnetic reconnection and related explosive phenomena as a fundamental plasma process.

physics.plasm-ph2020★ 2 cited

A drift-kinetic method for obtaining gradients in plasma properties from single-point distribution function data

Blake A. Wetherton, Jan Egedal, Peter K. Montag +2

In this paper, we derive a new drift-kinetic method for estimating gradients in the plasma properties through a velocity space distribution at a single point. The gradients are int…

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