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researcher

S. Boldyrev

8 papers hereh-index 222 citations8 works total

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

author position
  • first author1
  • middle author7

Across the 8 of 8 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE3
  • physics.plasm-ph3
  • astro-ph.GA1
  • astro-ph.SR1
same name
  • S. Boldyrev — 92 papers, h 36
  • S. Boldyrev — 4 papers, h 3
  • S. Boldyrev — 1 paper, h 4
  • S. Boldyrev — 1 paper, h 3
  • S. Boldyrev — 1 paper, h 2
  • S. Boldyrev — 1 paper, h 1

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
20192026
most citedExtreme Plasma Astrophysics

7 citations · 10 across the 7 of their papers we have counts for

collaborators
Showing 2026Show all

4 papers · 1 filter

physics.plasm-ph2026

Strong Nonlinear Alfvén Wave Interactions in a Laboratory Plasma

C. H. K. Chen, S. Dorfman, S. Boldyrev +6

Alfvén waves and their nonlinear interactions are ubiquitous in space and astrophysical plasmas, and are thought to play important roles in the dynamics of these systems, yet their…

astro-ph.HE2026

Particle acceleration in Alfvénic turbulence with a strong guide field

Daniel Humphrey, Stanislav Boldyrev, Vadim Roytershteyn

Magnetically dominated Alfvénic turbulence creates an effective environment for particle acceleration. However, when a strong mean field is present, traditional mechanisms like mir…

astro-ph.GA2026★ 1 cited

Particle acceleration and pitch-angle evolution in relativistic turbulence

Daniel Humphrey, Cristian Vega, Stanislav Boldyrev +1

Synchrotron radiation detected from relativistic astrophysical objects such as pulsar-wind nebulae and {jets from active galactic nuclei} depends on the magnetic fields and the dis…

astro-ph.HE2026

Whistler-Alfvén turbulence in a non-neutral ultrarelativistic pair plasma

Stanislav Boldyrev, Mikhail Medvedev

The large-scale dynamics of most conventional space and astrophysical plasmas are predominantly governed by Alfvén modes, which are low-frequency magnetohydrodynamic modes existing…

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