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researcher

M. Goldstein

29 papers hereh-index 6516.3k citations442 works total

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

author position
  • middle author14
  • last author8

Across the 22 of 29 papers where every author was matched, so the position is known.

fields
  • physics.space-ph12
  • astro-ph.SR10
  • physics.plasm-ph7
same name
  • M. Goldstein — 84 papers, h 24
  • M. Goldstein — 8 papers, h 33
  • M. Goldstein — 5 papers, h 2
  • M. Goldstein — 3 papers, h 3
  • M. Goldstein — 2 papers, h 11
  • M. Goldstein — 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
20092022
most citedScaling of the electron dissipation range of solar wind turbulence

164 citations · 1.2k across the 29 of their papers we have counts for

collaborators
Showing 2020 · physics.space-phShow all

3 papers · 2 filters

physics.space-ph2020★ 16 cited

Random Walk and Trapping of Interplanetary Magnetic Field Lines: Global Simulation, Magnetic Connectivity, and Implications for Solar Energetic Particles

Rohit Chhiber, David Ruffolo, William H. Matthaeus +4

The random walk of magnetic field lines is an important ingredient in understanding how the connectivity of the magnetic field affects the spatial transport and diffusion of charge…

physics.space-ph2020★ 6 cited

Major Scientific Challenges and Opportunities in Understanding Magnetic Reconnection and Related Explosive Phenomena in Solar and Heliospheric Plasmas

H. Ji, J. Karpen, A. Alt +105

Magnetic reconnection underlies many explosive phenomena in the heliosphere and in laboratory plasmas. The new research capabilities in theory/simulations, observations, and labora…

physics.space-ph2020★ 126 cited

Shear-Driven Transition to Isotropically Turbulent Solar Wind Outside the Alfven Critical Zone

D. Ruffolo, W. H. Matthaeus, R. Chhiber +11

Motivated by prior remote observations of a transition from striated solar coronal structures to more isotropic ``flocculated'' fluctuations, we propose that the dynamics of the in…

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