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researcher

V. Angelopoulos

64 papers hereh-index 8938.1k citations1.1k works total

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

author position
  • first author1
  • middle author44
  • last author16

Across the 61 of 64 papers where every author was matched, so the position is known.

fields
  • physics.space-ph45
  • physics.plasm-ph14
  • astro-ph.EP1
  • astro-ph.SR1
  • physics.geo-ph1
  • physics.ins-det1
same name
  • V. Angelopoulos — 5 papers, h 40
  • V. Angelopoulos — 4 papers, h 9
  • V. Angelopoulos — 3 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
20012026
most citedRelativistic electrons produced by foreshock disturbances

83 citations · 892 across the 63 of their papers we have counts for

collaborators
Showing 2018Show all

3 papers · 1 filter

physics.space-ph2018★ 22 cited

First results from sonification and exploratory citizen science of magnetospheric ULF waves: Long-lasting decreasing-frequency poloidal field line resonances following geomagnetic storms

M. O. Archer, M. D. Hartinger, R. Redmon +2

Magnetospheric ultra-low frequency (ULF) waves contribute to space weather in the solar wind - magnetosphere - ionosphere system. The monitoring of these waves by space- and ground…

physics.plasm-ph2018★ 61 cited

Evolution of electron distribution driven by nonlinear resonances with intense field-aligned chorus waves

D. Vainchtein, X. -J. Zhang, A. V. Artemyev +3

Resonant electron interaction with whistler-mode chorus waves is recognized as one of the main drivers of radiation belt dynamics. For moderate wave intensity, this interaction is…

physics.space-ph2018★ 52 cited

Dayside magnetospheric and ionospheric responses to a foreshock transient on June 25, 2008: 2. 2-D evolution based on dayside auroral imaging

Boyi Wang, Yukitoshi Nishimura, Heli Hietala +8

The foreshock region involves localized and transient structures such as foreshock cavities and hot flow anomalies due to solar wind-bow shock interactions, and foreshock transient…

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