Author/Authors :
Vasko، نويسنده , , I.Y. and Zelenyi، نويسنده , , L.M. and Artemyev، نويسنده , , A.V. and Petrukovich، نويسنده , , A.A. and Malova، نويسنده , , H.V. and Zhang، نويسنده , , T.L. and Fedorov، نويسنده , , A.O. and Popov، نويسنده , , V.Y. and Barabash، نويسنده , , S. and Nakamura، نويسنده , , R.، نويسنده ,
Abstract :
We investigate the current sheet (CS) of the Venusian magnetotail using the data collected by the Venus Express mission in 2006–2010. We have found that the observed profiles of the main magnetic field component Bx have single-scale or double-scale structures. For single-scale CSs the Bx profile is well approximated by the Harris model, B 0 tanh ( t / T 0 ) (T0 is the characteristic temporal scale, B0 is the magnetic field at the CS boundary). For double-scale CSs the Bx profile is better described by the double-scale model, B 1 tanh ( t / T 1 ) + B 2 tanh ( t / T 2 ) with B 2 > 0.3 B 0 and T 2 > 2 T 1 . The magnetic field component perpendicular to the CS plane and the shear component are on average uniform across CSs and ten times smaller than the amplitude of Bx. The observed Bx profiles can be described by the quasiadiabatic CS model. According to our interpretation the electric current in single-scale CSs is generally carried by protons on transient orbits. In double-scale CSs the current density is provided by transient protons and oxygen ions. In this case, the inner CS scale is supported by the proton population, while the outer scale is supported by the oxygen population. We suggest that the Venusian CS thickness is likely several ion thermal gyroradii.
