Abstract

The Visible Imaging System (VIS) is a set of three low-light-level cameras to be flown on the POLAR spacecraft of the Global Geospace Science (GGS) program which is an element of the International Solar-Terrestrial Physics (ISTP) campaign. Two of these cameras share primary and some secondary optics and are designed to provide images of the night-time auroral oval at visible wavelengths. A third camera is used to monitor the directions of the fields-of-view of these sensitive auroral cameras with respect to sunlit Earth. The auroral emissions of interest include those from N₂⁺ at 391.4 nm, OI at 557.7 and 630.0 nm, HI at 656.3 nm, and OII at 732.0 nm. The two auroral cameras have different spatial resolutions. These resolutions are about 10 km and 20 km from a spacecraft altitude of 8 R_e. The time to acquire and telemeter a 256 × 256-pixel image is about 12 s. The primary scientific objectives of this imaging instrumentation, together with the in situ observations from the ensemble of ISTP spacecraft, are (1) quantitative assessment of the dissipation of magnetospheric energy into the auroral ionosphere, (2) an instantaneous reference system for the in situ measurements, (3) development of a substantial model for energy flow within the magnetosphere, (4) investigation of the topology of the magnetosphere, and (5) delineation of the responses of the magnetosphere to substorms and variable solar wind conditions.