A Saturn Net Flux Radiometer (SNFR) is being developed as part of a payload for a future NASA-led Saturn Probe Mission. The current design has two spectral channels i.e., a solar channel (0.4-to-5 μm) and a thermal channel (4-to-50 μm). The SNFR is capable of viewing five distinct viewing angles during the descent. Non-imaging Winston cones with window and filter combinations define the spectral channels, each with a 5° field-of-view. Un - cooled thermopile detectors are used in each spectral channel and are read out using a custom-designed Application Specific Integrated Circuit (ASIC). The SNFR measures the radiative energy anisotropies with altitude. In the solar channel, the downward flux will determine the solar energy deposition profile and the upward flux will yield information about cloud particle absorption and scattering. In the thermal channel, the net flux will define sources and sinks of planetary radiation. In conjunction with calculated gas and particulate opacities, these observations will determine the atmosphere’s radiative balance.
Presently, the focal plane array, ASIC front-end electronics, and software are being integrated. Comprehensive radiometric performance testing will follow.