bandeau.png

Analyzing the AO operational behavior of non-sidereal tracking on the Thirty Meter Telescope using SysML
John Miles  1, *@  , Gelys Trancho  1@  , Lianqi Wang  1@  , Corinne Boyer  1@  , David Andersen  1@  , Glen Herriot  2@  , Brent Ellerbroek  1@  , Maximilian Vierlboeck  3@  , Robert Karban  3@  
1 : TMT International Observatory
100 W. Walnut Street, Suite 300, Pasadena, CA 91124 -  United States
2 : NRC Herzberg Astronomy and Astrophysics
5071 West Saanich Road, Victoria, BC, V9E 2E7 -  Canada
3 : Jet Propulsion Laboratory
4800 Oak Grove Drive, Pasadena, CA 91109-8099, USA -  United States
* : Corresponding author

We have modeled the functional and physical architecture, behavior, requirements, and parametric relationships through system-level simulation of observation workflows, using OMG's Systems Modeling Language (SysML), to validate use-case scenarios and verify timing requirements early in the life-cycle phase. This paper presents preliminary results for non-sidereal tracking scenarios, for LGS MCAO modes where the NFIRAOS pyramid wavefront sensor and the on-instrument wavefront sensors must hand off from one guide star to another. Operational modes and behavior are modeled using activity diagrams. Scenarios are captured primarily using sequence and activity diagrams. Verifiable requirements are formally captured using constraints on properties. This type of modeling can be particularly useful when investigating the effect of parallelizing or re-ordering sequence tasks.


Online user: 2 RSS Feed | Privacy
Loading...