SSUSI Mission Objectives
APL has built five SSUSI sensors for DMSP. These sensors are intended to provide a quantitative description of the state of the upper atmosphere and the aurora on a global basis. In order for the data to be of use to the user community, rapid, efficient, and accurate operational algorithms have been developed to convert the radiance observations into environmental parameters.
The SSUSI design reflects the operational need for the monitoring of global space weather as summarized in the Memorandum of the Joint Chiefs of Staff MJCS 154-86. This memo ranked environmental parameters in order of priority. Table 1 summarizes those parameters with priority ranking that SSUSI will measure.
|MJCS 154-86 Rank of SSUSI Environmental Parameters|
|5||Electron Density Profile|
|12||Neutral Number Density Profile|
|16||Solar Radiation (EUV integrated flux)|
|18||Auroral Emissions and Airglow|
|24||Precipitating Electrons and Ions|
The Far UV is ideally suited to determining thermospheric and ionospheric environmental parameters. It possesses optical signatures of all the major thermospheric species: O, N2, and O2 (O2 is seen in absorption on the limb) and the dominant F-region ion, O+ (on the nightside).