The Waves instrument aboard Juno is a sophisticated radio astronomy
observatory investigating Jupiter's auroral radio emissions and plasma
wave interactions. Waves records electrical field properties using two
monopole antennas, which are connected to form a dipole. The receiving
properties of the Waves dipole changes quite remarkably over the
instruments frequency range from near DC to 40 MHz. In this contribution
we outline Waves' electrical sensor properties above the quasi-static
frequency range and provide detailed directivity pattern and insertion
loss figures of the instrument for science application and data
analysis.