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                   210                       MEMS and Microstructures in Aerospace Applications


                   rotated, Coriolis forces cause the sense mass to oscillate out of plane. This change is
                   measured by capacitive plates and is proportional to the rotational rate of the body.
                       The MEMS three-axis gyro sub-assembly used in the SC is depicted in
                   Figure 10.2. The specific MEMS inertial sensing instrument used in the ISC is
                   the TFG14-R3, 20-mm thick gyro fabricated in a silicon-on-insulator process that
                   incorporates novel features for high performance. Under typical operating condi-
                   tions, the MEMS gyroscopes drive the ISC output attitude. The MEMS gyros
                   sensed inertial rates are sampled, at the high sample frequency of 100 Hz, by the
                   embedded flight processor. The raw gyro data are then processed using a Kalman
                   filter algorithm to produce the estimated reference attitude quaternion, which is
                   communicated to the host spacecraft in real time, at a frequency of 5 Hz. The APS
                   star camera is used periodically (every few minutes) to obtain a camera quaternion,
                   whose main purpose is to compensate the inherent drift of the gyros. A simple
                   system data flow is shown in Figure 10.3.
                       A typical profile of attitude error, computed by simulation, is shown in
                   Figure 10.4. The 1-sigma error bounds are shown in bold, while the actual attitude
                   error from one simulated run is shown as a thin line. Since the error bounds are
                   1-sigma, the error can be expected to go outside of the bound for 32% of the time.
                   Every 5 min, the gyros are compensated with a fresh star camera quaternion, as
                   evidenced by the sudden narrowing of the error bounds. Used together as a tightly
                   integrated sensor suite, the MEMS gyros and star camera enhance each other’s




                                  Gyro data
                                   ∆θ Pulses   Gyro acquisition
                                    Temp           100 Hz
                                                   Gyro
                                                compensation
                                    Compensation
                                                      High frequency
                                                ECI quaternion
                                                determination     Attitude
                                                      Low frequency controllers
                                                      Request at 50 Hz
                                                  Kalman
                                                   filter
                                              (Square root type
                                               with 27 states)
                                 Camera data
                                                           Time stamped
                                            Img. processing
                                     Star     and attitude  quaternion from
                                   images                  camera processing
                                             determination
                   FIGURE 10.3 NMP ST6 ISC attitude determination system data flow. (Source: NASA
                   CALTECH/JPL.)




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