Sandra C. Chapman

发表

Quantifying scaling in the velocity field of the anisotropic turbulent solar wind

S. Chapman, B. Hnat, Sandra C. Chapman, 2007 .

Kinetic equation of linear fractional stable motion and applications to modeling the scaling of intermittent bursts.

R. Sánchez, N. Watkins, D. Credgington, 2008, Physical review. E, Statistical, nonlinear, and soft matter physics.

Scale-free texture of the fast solar wind.

S C Chapman, R. Wicks, S. Chapman, 2011, Physical review. E, Statistical, nonlinear, and soft matter physics.

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

R. M. Nicol, S. Chapman, B. Hnat, 2007, Physical review letters.

TURBULENT CHARACTERISTICS IN THE INTENSITY FLUCTUATIONS OF A SOLAR QUIESCENT PROMINENCE OBSERVED BY THE HINODE SOLAR OPTICAL TELESCOPE

S. Chapman, C. Foullon, S. Chapman, 2011, 1110.3159.

Scaling collapse and structure functions: identifying self-affinity in finite length time series

N. Watkins, G. Rowlands, S. Chapman, 2005, physics/0504024.

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

G. Rowlands, S. Chapman, B. Hnat, 2004, physics/0412063.

On the fractal nature of the magnetic field energy density in the solar wind

N. Watkins, G. Rowlands, S. Chapman, 2007 .

Kinetic signatures and intermittent turbulence in the solar wind plasma.

W. Matthaeus, S. Chapman, B. Hnat, 2012, Physical review letters.

Identification of intermittent multifractal turbulence in fully kinetic simulations of magnetic reconnection.

H. Karimabadi, V. Roytershteyn, S. Chapman, 2013, Physical review letters.

Nonaxisymmetric anisotropy of solar wind turbulence as a direct test for models of magnetohydrodynamic turbulence.

A. Turner, Sandra C. Chapman, Grigol Gogoberidze, 2011, Physical review letters.