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P. Dmitruk

36 papers hereh-index 394.9k citations140 works total

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

author position
  • first author5
  • middle author19
  • last author12

Across the 36 of 36 papers where every author was matched, so the position is known.

fields
  • physics.plasm-ph13
  • physics.flu-dyn7
  • physics.space-ph6
  • astro-ph4
  • astro-ph.SR3
  • physics.comp-ph2
same name
  • P. Dmitruk — 7 papers, h 5
  • P. Dmitruk — 6 papers

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
19972025
most citedA turbulence-driven model for heating and acceleration of the fast wind in coronal holes

234 citations · 1.3k across the 36 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

3 papers · 1 filter

astro-ph.SR2022★ 18 cited

A Statistical Study of the Compressible Energy Cascade Rate in Solar Wind Turbulence: Parker Solar Probe Observations

Maia Brodiano, Pablo Dmitruk, Nahuel Andrés

We investigated incompressible and compressible magnetohydrodynamic (MHD) energy cascade rates in the solar wind at different heliocentric distances. We used in situ magnetic field…

astro-ph.SR2014★ 49 cited

Test-particle acceleration in a hierarchical three-dimensional turbulence model

S. Dalena, A. F. Rappazzo, P. Dmitruk +2

The acceleration of charged particles is relevant to the solar corona over a broad range of scales and energies. High-energy particles are usually detected in concomitance with lar…

astro-ph.SR2009★ 234 cited

A turbulence-driven model for heating and acceleration of the fast wind in coronal holes

A. Verdini, M. Velli, W. H. Matthaeus +2

A model is presented for generation of fast solar wind in coronal holes, relying on heating that is dominated by turbulent dissipation of MHD fluctuations transported upwards in th…

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