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researcher

G. Howes

65 papers hereh-index 395.3k citations171 works total

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

author position
  • sole author8
  • first author15
  • middle author33
  • last author7

Across the 63 of 65 papers where every author was matched, so the position is known.

fields
  • physics.plasm-ph23
  • astro-ph.SR21
  • physics.space-ph12
  • astro-ph7
  • astro-ph.EP1
  • astro-ph.HE1
same name
  • G. Howes — 23 papers, h 12

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 citedMagnetic fluctuation power near proton temperature anisotropy instability thresholds in the solar wind

468 citations · 4.8k across the 64 of their papers we have counts for

collaborators
Showing 2012 · physics.space-phShow all

3 papers · 2 filters

physics.space-ph2012★ 21 cited

Kinetic Scale Density Fluctuations in the Solar Wind

C. H. K. Chen, G. G. Howes, J. W. Bonnell +3

We motivate the importance of studying kinetic scale turbulence for understanding the macroscopic properties of the heliosphere, such as the heating of the solar wind. We then disc…

physics.space-ph2012★ 104 cited

Using Synthetic Spacecraft Data to Interpret Compressible Fluctuations in Solar Wind Turbulence

K. G. Klein, G. G. Howes, J. M. TenBarge +3

Kinetic plasma theory is used to generate synthetic spacecraft data to analyze and interpret the compressible fluctuations in the inertial range of solar wind turbulence. The kinet…

physics.space-ph2012★ 65 cited

Interpreting Magnetic Variance Anisotropy Measurements in the Solar Wind

J. M. TenBarge, J. J. Podesta, K. G. Klein +1

The magnetic variance anisotropy (Am​) of the solar wind has been used widely as a method to identify the nature of solar wind turbulent fluctuations; however, a thorou…

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