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Sandra C. Chapman

3 papers hereh-index 15925 citations18 works total

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

author position
  • middle author3

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • cs.DC1
  • physics.plasm-ph1
  • physics.space-ph1
same name
  • Sandra C. Chapman — 1 paper, h 2

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
20072026
most citedSelf-similar signature of the active solar corona within the inertial range of solar wind turbulence

45 citations · 46 across the 3 of their papers we have counts for

collaborators

3 papers

physics.plasm-ph2026

A tensor invariant approach to energy flux in magnetohydrodynamic turbulence

Conan M. Liptrott, Sandra C. Chapman, Bogdan Hnat +1

A scale-by-scale analysis of energy flux in the turbulent cascade can be performed using the spatially filtered magnetohydrodynamic (MHD) equations, while the gradient tensor invar…

cs.DC2016★ 1 cited

A parallel workload has extreme variability

R. Henwood, N. W. Watkins, S. C. Chapman +1

In both high-performance computing (HPC) environments and the public cloud, the duration of time to retrieve or save your results is simultaneously unpredictable and important to y…

physics.space-ph2007★ 45 cited

Self-similar signature of the active solar corona within the inertial range of solar wind turbulence

K. Kiyani, S. C. Chapman, B. Hnat +1

We quantify the scaling of magnetic energy density in the inertial range of solar wind turbulence seen in-situ at 1AU with respect to solar activity. At solar maximum, when the cor…

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