  The Juno Orbiter is measuring the three-dimensional gravity field
perturbation of Jupiter induced by its rapid rotation, zonal flows, and tidal
response to its major natural satellites. This paper aims to provide the
contributions to the tesseral harmonics coefficients Cnm, Snm, and the Love
numbers knm to be expected from static tidal response in the gravity field of
rotating Jupiter. For that purpose, we apply the method of Concentric Maclaurin
Ellipsoids (CMS). As we are interested in the variation of the tidal potential
with the longitudes of the moons, we take into account the simultaneous
presence of the satellites Io, Europa, and Ganymede. We assume co-planar,
circular orbits with normals parallel to Jupiter's spin axis. The
planet-centered longitude of Io in the three-moon case is arbitrarily assumed
varphi = 0. Under these assumptions we find maximum amplitudes and fluctuations
of 3.5 times 10^-8 +- 15% for C22. For the Love numbers, largest variation of
10% to 20% is seen in k42 and k62, whereas the values k2, k33, and k44 fall
into narrow ranges of 0.1% uncertainty or less. In particular, we find
k2=k2,Io(1 +- 0.02%) where k2,Io=0.5897 is the static tidal response to lone
Io. Our obtained gravity field perturbation leads to a maximum equatorial shape
deformation of up to 28m. We suggest that should Juno measurements of the knm
deviate from those values, it may be due to dynamic or dissipative effects on
Jupiter's tidal response. Finally, an analytic expression is provided to
calculate the tesseral harmonics contribution from static tidal response for
any configuration of the satellites.
