activity
20072013
most citedSelf-similar signature of the active solar corona within the inertial range of solar wind turbulence

45 citations · 106 across the 5 of their papers we have counts for

collaborators

5 papers

physics.plasm-ph2013★ 9 cited

Identifying low-dimensional dynamics in Type-I edge-localised-mode processes in JET plasmas

F. A. Calderon, R. O. Dendy, S. C. Chapman +4

Edge localised mode (ELM) measurements from reproducibly similar plasmas in the Joint European Torus (JET) tokamak, which differ only in their gas puffing rate, are analysed in ter…

physics.plasm-ph2009★ 13 cited

Generalized similarity in finite range solar wind magnetohydrodynamic turbulence

S. C. Chapman, R. M. Nicol

Extended or generalized similarity is a ubiquitous but not well understood feature of turbulence that is realized over a finite range of scales. ULYSSES spacecraft solar polar pass…

astro-ph.SR2009★ 18 cited

Quantifying the Anisotropy and Solar Cycle Dependence of "" Solar Wind Fluctuations Observed by Ace

R. M. Nicol, S. C. Chapman, R. O. Dendy

The power spectrum of the evolving solar wind shows evidence of a spectral break between an inertial range of turbulent fluctuations at higher frequencies and a "" like region…

astro-ph2007★ 21 cited

The signature of evolving turbulence in quiet solar wind as seen by ULYSSES

R. M. Nicol, S. C. Chapman, R. O. Dendy

Solar wind fluctuations, such as magnetic field or velocity, show power law power spectra suggestive both of an inertial range of intermittent turbulence (with exponent…

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…