Mapping Mercury's internal magnetic field with a magnetometer in closed orb
it around the planet will provide valuable information about its internal s
tructure. By measuring magnetic field multipoles of order higher than the d
ipole we could, in principle, determine some properties, such as size and l
ocation, of the internal source. Here we try to quantify these expectations
. Using conceptual models, we simulate the actual measurement during the Be
piColombo mission, and then we analyze the simulated data in order to estim
ate the measurement errors due to the limited spatial sampling. We also inv
estigate our ability to locate the field generating current system within t
he planet. Finally, we address the main limitation of our model, due to the
presence of time-varying external magnetospheric currents. (C) 2001 Publis
hed by Elsevier Science Ltd.