Kinetic‐Scale Turbulence in the Venusian Magnetosheath
Open Access
- 18 January 2021
- journal article
- research article
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 48 (2)
- https://doi.org/10.1029/2020gl090783
Abstract
No abstract availableThis publication has 96 references indexed in Scilit:
- The Solar Wind as a Turbulence LaboratoryLiving Reviews in Solar Physics, 2013
- SIMULATIONS OF ELECTRON MAGNETOHYDRODYNAMIC TURBULENCEThe Astrophysical Journal, 2009
- Giant vortices lead to ion escape from Venus and re‐distribution of plasma in the ionosphereGeophysical Research Letters, 2009
- Dissipation in Turbulent Plasma due to Reconnection in Thin Current SheetsPhysical Review Letters, 2007
- Solar wind proton temperature anisotropy: Linear theory and WIND/SWE observationsGeophysical Research Letters, 2006
- Finite size scaling in the solar wind magnetic field energy density as seen by WINDGeophysical Research Letters, 2002
- Intermittency in the solar wind turbulence through probability distribution functions of fluctuationsGeophysical Research Letters, 1999
- Observational constraints on the dynamics of the interplanetary magnetic field dissipation rangeJournal of Geophysical Research, 1998
- Non-Gaussian statistics in space plasma turbulence: fractal properties and pitfallsNonlinear Processes in Geophysics, 1996
- WAVELET TRANSFORMS AND THEIR APPLICATIONS TO TURBULENCEAnnual Review of Fluid Mechanics, 1992