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researcher

T. Bowen

58 papers hereh-index 263.3k citations91 works total

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

author position
  • first author10
  • middle author37

Across the 47 of 58 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR32
  • physics.space-ph18
  • physics.plasm-ph5
  • astro-ph.IM1
  • eess.SP1
  • physics.ins-det1
same name
  • T. Bowen — 2 papers, h 2
  • T. Bowen — 1 paper, h 6

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
20132026
most citedThe Evolution and Role of Solar Wind Turbulence in the Inner Heliosphere

270 citations · 2.3k across the 58 of their papers we have counts for

collaborators
Showing 2024 · astro-ph.SRShow all

4 papers · 2 filters

astro-ph.SR2024

Extended Cyclotron Resonant Heating of the Turbulent Solar Wind

Trevor A. Bowen, Ivan Y. Vasko, Stuart D. Bale +8

Circularly polarized, nearly parallel propagating waves are prevalent in the solar wind at ion-kinetic scales. At these scales, the spectrum of turbulent fluctuations in the solar…

astro-ph.SR2024★ 11 cited

Near subsonic solar wind outflow from an active region

Tamar Ervin, Stuart D. Bale, Samuel T. Badman +10

During Parker Solar Probe (Parker) Encounter 15 (E15), we observe an 18-hour period of near subsonic (MS​∼ 1) and sub-Alfvénic (SA), MA​ <<< 1, slow speed…

astro-ph.SR2024★ 9 cited

Dominance of 2-Minute Oscillations near the Alfvén Surface

Zesen Huang, Marco Velli, Chen Shi +11

Alfvén waves, considered one of the primary candidates for heating and accelerating the fast solar wind, are ubiquitous in spacecraft observations, yet their origin remains elusive…

astro-ph.SR2024

Resonance of low-frequency electromagnetic and ion-sound modes in the solar wind

I. Y. Vasko, F. S. Mozer, T. Bowen +6

Parker Solar Probe measurements have recently shown that coherent fast magnetosonic and Alfvén ion-cyclotron waves are abundant in the solar wind and can be accompanied by higher-f…

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