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most citedMagnetic Reconnection and Intermittent Turbulence in the Solar Wind

174 citations · 665 across the 23 of their papers we have counts for

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physics.space-ph2014★ 174 cited

Magnetic Reconnection and Intermittent Turbulence in the Solar Wind

K. T. Osman, W. H. Matthaeus, J. T. Gosling +5

A statistical relationship between magnetic reconnection, current sheets and intermittent turbulence in the solar wind is reported for the first time using in-situ measurements fro…

physics.space-ph2013★ 31 cited

Proton Kinetic Effects and Turbulent Energy Cascade Rate in the Solar Wind

Kareem T. Osman, William H. Matthaeus, Khurom H. Kiyani +2

The first observed connection between kinetic instabilities driven by proton temperature anisotropy and estimated energy cascade rates in the turbulent solar wind is reported using…

physics.space-ph2011★ 14 cited

The scale-free texture of the fast solar wind

B. Hnat, S. C. Chapman, G. Gogoberidze +1

The higher order statistics of magnetic field magnitude fluctuations in the fast quiet solar wind are quantified systematically scale-by-scale for the first time. We find a single…

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…

physics.space-ph2004★ 47 cited

Scaling and a Fokker-Planck model for fluctuations in geomagnetic indices and comparison with solar wind epsilon as seen by WIND and ACE

B. Hnat, S. C. Chapman, G. Rowlands

The evolution of magnetospheric indices on temporal scales shorter than that of substorms is characterized by bursty, intermittent events that may arise from turbulence intrinsic t…

physics.space-ph2002★ 28 cited

Scaling of solar wind epsilon and the AU, AL and AE indices

B. Hnat, S. C. Chapman, G. Rowlands +2

We apply the finite size scaling technique to quantify the statistical properties of fluctuations in AU, AL and AE indices and in the epsilon parameter that represents energy input…