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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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