The spacecraft wake: Interference with electric field observations and a possibility to detect cold ions

TL;DR

This paper reviews spacecraft wake effects on electric field measurements, presents models and statistics, and explores how wakes can be used to detect cold ions, especially in magnetospheric lobes.

Contribution

It provides a comprehensive analysis of wake phenomena, compares observations with models, and introduces a method to estimate cold ion fluxes using wake characteristics.

Findings

Wake effects vary with plasma environment and spacecraft charging.

Wakes can be used to estimate cold ion outflow from Earth.

Analytical models align with observed wake statistics.

Abstract

Wakes behind spacecraft caused by supersonic drifting positive ions are common in plasmas and disturb in situ measurements. We review the impact of wakes on observations by the Electric Field and Wave double-probe instruments on the Cluster satellites. In the solar wind, the equivalent spacecraft charging is small compared to the ion drift energy and the wake effects are caused by the spacecraft body and can be compensated for. We present statistics of the direction, width, and electrostatic potential of wakes, and we compare with an analytical model. In the low-density magnetospheric lobes, the equivalent positive spacecraft charging is large compared to the ion drift energy and an enhanced wake forms. In this case observations of the geophysical electric field with the double-probe technique becomes extremely challenging. Rather, the wake can be used to estimate the flux of cold (eV) positive ions. For an intermediate range of parameters, when the equivalent charging of the spacecraft is similar to the drift energy of the ions, also the charged wire booms of a double-probe instrument must be taken into account. We discuss an example of these effects from the MMS spacecraft near the magnetopause. We find that many observed wake characteristics provide information that can be used for scientific studies. An important example is the enhanced wakes used to estimate the outflow of ionospheric origin in the magnetospheric lobes to about ${10}^{26}$ cold (eV) ions/s, constituting a large fraction of the mass outflow from planet Earth.