Plasma Instrument for Magnetic Sounding
The Plasma Instrument for Magnetic Sounding is a Faraday cup based instrument that will fly on board the Europa Clipper orbiter to explore Jupiter's moon Europa. PIMS will measure the plasma that populates Jupiter's magnetosphere and Europa's ionosphere.
The Principal investigator is Joseph Westlake, from the Johns Hopkins University Applied Physics Laboratory.
Overview
The plasma in Jupiter's magnetosphere interacts with Europa's atmosphere. This interaction results in magnetic field perturbations. While understanding this plasma interaction is inherently interesting, it is also crucial for successful magnetic sounding Europa's subsurface ocean. The interaction of the Jovian magnetic field with Europa's subsurface ocean produces a magnetic induction signature that is used to determine the ice shell thickness, ocean depth, and ocean salinity of Europa's subsurface ocean. Separating the sources of magnetic field perturbations produces a better understanding of the ocean's properties.The Plasma Instrument for Magnetic Sounding is a Faraday cup-based instrument that will measure the plasma of Jupiter's magnetosphere and Europa's ionosphere. Such devices on spacecraft date back to Explorer 10 in 1961 and were used by the Voyager 1 spacecraft to study Jupiter's magnetosphere in 1979.
Science goals
The three science goals of PIMS investigation are:- study how Europa influences its magnetosphere, and Jupiter's magnetosphere.
- study the mechanisms for weathering and releasing material from Europa's surface into the atmosphere and ionosphere.
- constrain the inner ocean's salinity and depth.
Principle
In the Jovian magnetospheric plasma PIMS measures the density and flow velocity of ions with energies below 7 keV, and the density and energy of electrons with energies below 2 keV. In Europa's ionosphere PIMS measures the density and temperature of ions and electrons. The PIMS investigation can also help in the search for active plumes and measure their mass-loading, by measuring the magnetic perturbations of Europa's ionosphere.
PIMS works in synergy with the Interior Characterization of Europa using Magnetometry instrument to probe Europa's subsurface ocean.
Parameter | Performance |
In Magnetospheric Mode | •Electron energy: 10 eV – 2 keV •Ion energy: 20 eV – 6 keV |
In Ionospheric Mode | •Electron energy: 1 – 50 eV •Ion energy: 1 – 50 eV |
Energy resolution | 10% ΔE/E |
Sensitivity | 0.5 pA/cm2 – 1×105 pA/cm2 |
Field of view | 4 × 90° cone |
Temporal resolution | 1 second for a full ion and electron sweep in Ionospheric Mode 4 seconds for a full ion and electron sweep in Magnetospheric Mode 5 seconds for a full ion and electron sweep in Transition Mode |