Mesogranulation and Turbulence in Photospheric Flows
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[1] D. Hathaway,et al. The Photospheric Convection Spectrum , 2000 .
[2] R. Shine,et al. Supergranule and Mesogranule Evolution , 2000 .
[3] A. Ruzmaikin,et al. Characteristic Scales of Photospheric Flows and Their Magnetic and Temperature Markers , 1999 .
[4] A. Ruzmaikin,et al. Spatiotemporal Correlations and Turbulent Photospheric Flows from SOHO/MDI Velocity Data , 1998 .
[5] R. Kitai,et al. 3D Velocity-Field Observation of Solar Convection I. Characteristics of Mesogran , 1998 .
[6] C. Cadavid,et al. Spectral Properties of Solar Convection and Diffusion , 1996 .
[7] C. J. Wolfson,et al. The Solar Oscillations Investigation - Michelson Doppler Imager , 1995 .
[8] C. Basdevant,et al. Wavelet spectra compared to Fourier spectra , 1995 .
[9] D. Chou,et al. Power Spectra of Median- and Small-Scale Solar Convection , 1992 .
[10] G. Simon,et al. On the evidence for mesogranules in solar power spectra , 1992 .
[11] T. Duvall,et al. Power spectra of solar convection , 1991 .
[12] N. Weiss,et al. Simulation of Large-Scale Flows at the Solar Surface , 1989 .
[13] P. Holmes,et al. Turbulence, Coherent Structures, Dynamical Systems and Symmetry: THE BOUNDARY LAYER , 1996 .
[14] M. Farge. Wavelet Transforms and their Applications to Turbulence , 1992 .
[15] F. Deubner. Mesogranulation: a convective phenomenon , 1989 .