Abstract
We have surveyed the Voyager 1 and 2 spacecraft magnetic field data from launch in 1977 through 1990 using daily spectrograms to find suitably long data intervals and to eliminate times near transients or strong gradients that might not represent homogeneous turbulence intervals. In the process, we have also omitted times when waves due to suprathermal particle populations such as interstellar pickup ions can be seen. Our goal was to construct a database of interplanetary magnetic field spectra that could be used in our companion papers to study the properties of the inertial and dissipation range of interplanetary turbulence. Here, we list those data intervals along with their heliocentric distance, latitude, and longitude as well as the angle between the mean magnetic field and the radial direction. Furthermore, we show the mean plasma parameters for the intervals listed. We invite others to use these listings in their associated studies.
