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The TRACE Model for Operations

The TRACE Model for Operations. Ted Tarbell tarbell@lmsal.com. The TRACE Model for Operations. TRACE Initial Phases Transition to Long-Term Operational Phase Why TRACE Remote Operations Works Tools for TRACE Planners & Monitors Science Coordination with Remote Planners

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The TRACE Model for Operations

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  1. The TRACE Model for Operations Ted Tarbell tarbell@lmsal.com

  2. The TRACE Model for Operations • TRACE Initial Phases • Transition to Long-Term Operational Phase • Why TRACE Remote Operations Works • Tools for TRACE Planners & Monitors • Science Coordination with Remote Planners • Report on Other Missions by Dr. Chuck Holmes (NASA HQ) T. D. Tarbell, LMSAL tarbell@lmsal.com

  3. TRACE Initial Phase (1) • Launch (2 April, 1998) to 1st eclipse season (November, 1998) • April: 3 weeks outgassing, 1 week engineering checkout • May - June: 6 weeks to finish “Initial 30-Day Plan,” coordinated with SOHO • June – November: 5 months of observing without SOHO, refining observing programs and procedures, and training weekly science planners • All Operations at GSFC Experiment Operations Facility • No instrument problems so engineering staff went home after ~1 week • 2 scientists, 1 assistant, 1 computer sysadmin resident at GSFC • All other weekly planners traveled to GSFC for 7-10 day visits • Science planning by telecons and lots of email • Daily telecons at first with LMSAL/SAO/MSU, then weekly • Simple coordinations with Yohkoh & ground based observatories

  4. TRACE Initial Phase (2) • All science observing programs were completely rewritten in this period • Better types of sequences were developed, both for science and for calibration • Most preflight sequences were never used again • Operations were difficult for the early planners • Only ~6 people had enough knowledge of the instrumdent to be a weekly planner, learning how to do it on the job • Much stress from daily deadlines and too many details to follow • When operations began to settle down shortly before eclipse season, we began to train new planners • Science Planning & Operations in this phase were done with approximately the same approach as that of the Solar-B MODA Outline

  5. Transition to Operational Phase • During 1st eclipse season, planning software installed at LMSAL • Mirroring of planning data, ftp transfers of timelines and quick look data completely successful • During 2nd year of observing, 2 scientists, 1-2 assistant planners, 1 computer sysadmin resident at GSFC • Occasional visits by other scientists to be weekly planner • Frequent JOP’s with SOHO scientists at GSFC and in France • After 2nd year, no resident scientists, 1 part-time planner, 1 part-time computer sysadmin • Most planning now done at LMSAL, SAO, MSU • Travel to GSFC is done by choice to interact with scientists there, not by necessity to do science planning & operations

  6. Why TRACE Remote Operation Works • Science planning is done by email & telecon, even daily target selection • Observing programs are always prepared in advance, and usually tested onboard before a JOP is run with other instruments • Planning data (SAA’s, station passes, etc.) and quick-look telemetry is mirrored to multiple remote sites (LMSAL, MSU, SAO) • Remote sites run same planning software as in GSFC EOF • Prepare observing tables & timelines, send to GSFC by secure sftp and ssh for uplink by the NASA satellite operators • No normal Real-Time operations except uplink of timeline and tables • People watch web displays of health & status at different places & times • One part-time science planner at GSFC always on-call

  7. TRACE Timeline Generator / Editor Header Editor Timeline Editor Current onboard Obs. Sequences

  8. TRACE Target Selector Main Widget Past location in blue, Future locations in green, Squares for TRACE & MDI HiRES FOV’s

  9. TRACE Simulator TRACE Simulator

  10. Web Health Monitoring

  11. Observation As-Run Summary

  12. TRACE Sequences & Frames

  13. TRACE Frame Generator / Editor main widget frame files CCD areas

  14. Science Coordination with Remote Planners • TRACE has run successful joint observations not only with SOHO at GSFC but also with: • SOHO “MEDOC Campaigns” with planners in Paris • Ground-based observatories in the Canary Islands, Sac Peak & Hawaii • Yohkoh and ground-based observatories in Japan • Campaigns must be scheduled well in advance • Observing programs must be written and run on simulator in advance • Usually tested onboard by a short run a few days in advance • All parties must understand & follow the timing constraints for target selection • All email must go to trace_planner (NOT to an individual person) because several people follow it in addition to the weekly planner

  15. SOHO Calendar

  16. Comments on Observing Table & Timeline Generation Tools • Need fast, local tools with intuitive GUI interfaces for use at ISAS • Need ability for remote scientists to make & test observing tables before coming to or sending them to ISAS, using nearly identical tools • Need developmental databases of observing tables and secure, “checked-in” database of observing tables approved for use in flight • Need simulator or compiler to validate observing tables before they are “checked in” • Access via the network for all of the developmental tools should be considered while designing the interfaces • Running locally using mirrored databases and/or running over the network, perhaps with reduced use of graphics to speed connectivity • Must guarantee adequate security, of course

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