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A feasible design for a magnetic diagnostics subsystem for eLISA will bebased on that of its precursor mission, LISA Pathfinder. Previous experienceindicates that magnetic field estimation at the positions of the test masseshas certain complications. This is due to two reasons. The first one is thatmagnetometers usually back-act due to their measurement principles (i.e., theyalso create their own magnetic fields), while the second is that the sensorsselected for LISA Pathfinder have a large size, which conflicts with spaceresolution and with the possibility of having a sufficient number of them toproperly map the magnetic field around the test masses. However,high-sensitivity and small-size sensors that significantly mitigate the twoaforementioned limitations exist, and have been proposed to overcome theseproblems. Thus, these sensors will be likely selected for the magneticdiagnostics subsystem of eLISA. Here we perform a quantitative analysis of thenew magnetic subsystem, as it is currently conceived, and assess thefeasibility of selecting these sensors in the final configuration of themagnetic diagnostic subsystem.

Interpolation of the magnetic field at the test masses in eLISA