Sagamihara Near Real-Time Fringe Detector to VSOG
GBTS Near Real-Time Fringe Detector to VSOG
What: During the mission, it will be necessary to have periodic and quick checks of the SRT performance using the near real-time fringe detectors at Usuda, Sagamihara and Green Bank. These single baseline correlators will provide prompt checks of the satellite's health. Delays and delay rates will be made available, together with details of the orbit used, to correlators and navigation teams.
How: TBD
When: Results reported within TBD days of the observation.
Where: TBD