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Correlation Length as a Function of B-V Angle

Global Quantities in Solar Wind Turbulence: Effect of B-V Angle and Averaging Interval. Jeffrey Tessein, Joshua Isaacs, and William Matthaeus University of Delaware, Newark, DE. Session: The dissipation of solar wind turbulence. Correlation Length as a Function of B-V Angle.

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Correlation Length as a Function of B-V Angle

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  1. Global Quantities in Solar Wind Turbulence: Effect of B-V Angle and Averaging Interval Jeffrey Tessein, Joshua Isaacs, and William Matthaeus University of Delaware, Newark, DE Session: The dissipation of solar wind turbulence. Correlation Length as a Function of B-V Angle • B-V angle is the angle between the velocity and mean magnetic field • Effect of B-V angle on cross helicity, Alfvén ratio, and correlation length • Effect of averaging interval on cross helicity, Alfvén ratio, and correlation length

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