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