Using magnetic helicity to diagnose wave vector direction in solar wind turbulence.
Robert T Wicks1, Daniel Verscharen1, Lloyd David Woodham2 and Miriam A Forman3, (1)University College London, Mullard Space Science Laboratory, London, United Kingdom, (2)Imperial College, London, United Kingdom, (3)Dept of Physics & Astronomy, Stony Brook, NY, United States
