Presentation is loading. Please wait.

Presentation is loading. Please wait.

1 Mission preparation Fred Lahuis SRON / Leiden Observatory MIRI NL Meeting ASTRON, 3 th June 2010.

Similar presentations


Presentation on theme: "1 Mission preparation Fred Lahuis SRON / Leiden Observatory MIRI NL Meeting ASTRON, 3 th June 2010."— Presentation transcript:

1 1 Mission preparation Fred Lahuis SRON / Leiden Observatory MIRI NL Meeting ASTRON, 3 th June 2010

2 2 Introduction Calibration Software development Operations Proposals Scheduling and commanding

3 3 Calibration Instrument calibration is a continuous effort -all through the mission preparation phase and the mission -FM test data will be used to obtain best possible pre-flight calibration -calibration goes hand-in-hand with software development FM test campaign is not designed to supply full instrument calibration -main purpose is verifying instrument requirements -will try to optimize/include test observations for calibration -however make sure things which cannot be done in-orbit are included -in parallel thinking about in-orbit commissioning has started -in part to screen FM performance tests FM delivery (data pack) is not a full FM calibration -contains some calibration files -calibration will be done after delivery An excellent instrument deserves an even better calibration

4 4 Software – EC history First EC software meetings in 2005 and 2006 -focussed on long-term plans for calibration and science analysis software Simulator developments 2006 and beyond -MTSSim at CSIC and SpecSim at ATC Meeting between EC and STScI at ATC in 2008 -followed by a visit of FL to STScI later in the year -collaboration agreement Jan 2010 MIRI EC software planning meeting -scope resources and work -strong focus on simulator development -planning for (pipeline related) Python development April 2010 first joint EC-STScI developers meeting at SRON Groningen Fred Lahuis coordinates EC development and is the main contact with STScI

5 5 Software – STScI history Very much in the planning stage Initial developments started -writing plans -some pipeline coding -studies, e.g. cosmic ray test 4 fte in 2010 -TBS how much later on -for all JWST instruments -support from STScI MIRI science team -e.g. plans, requirements, testing JWST Calibration Pipeline IRR and walk-through: June 10 DMS Requirements review: Autumn 2010

6 6 Software - simulators Strong need for simulator development -essential for instrument verification -required for Science and Calibration -provide test data for software development -SpecSim and MTSSim require upgrades -no simulators for Imager, LRS, Coronograpghs, detectors Simulator responsibility -SpecSim - UK-ATC -Coronograph - France / CEA -LRS - Germany MPIA/Cologne (+ France)‏ -Imager - France -SCA - UK-ATC -MTS – CSIC Spain

7 7 Software – Python development Collaborative effort of STScI and EC -no commitments from other teams yet Pipeline, calibration and science analysis -STScI focuses on pipeline -EC focuses on calibration and science analysis -mutual interest, expertise and support Distributed development -core python libraries defined -common JWST repository open to the EC -located outside STScI -maintained by the software team and not by STScI system management -developing ideas for tests, QA and developers guidelines

8 8 Software – near future Strong focus on simulators -upgrades this autumn in time for FM test preparations Software development plans -this year Stay in close contact with STScI -e.g. FL will attend STScI meetings Second joint developers meeting -likely attached to DMS meeting at STScI Initial Python coding -STScI/EC -Setup distributed development -STScI -basic imaging pipeline -EC -calibration analysis (initially tests developers are involved in)

9 9 Operations STScI (together with instrument teams) started preparations for mission operations Multiple Working Groups -JWST Science Working Group (BB) -MIRI-OWG with EC and NL (BB, SK and FL) participation -.... MIRI instrument team and STScI are preparing MIRI calibration plan -describes full analysis and calibration for the pipeline MIRI-OWG is preparing the MIRI Operations Concept Document -requires and initiates many detailed studies

10 10 Proposals STScI is mostly a general user mission -limited guaranteed time observations (GTO) -~10% over first 5 years -general observer (GO) proposals undergo standard TAC review -1 st year 50/50 GTO/GO -Additionally 5% for directors discretionary time (DDT) and targets of opportunity (ToO) STScI are designing new proposal preparation tool (PPT) -goal is to have a single phase proposal submission -at least for the bulk of the proposals -requires advanced PPT

11 11 Scheduling and commanding L2 makes scheduling easier -orbit puts less (absolute) time constraints on scheduling Scheduling will be optimized to: -minimize momentum build-up -> save fuel -> longer lifetime -maximize time usage -> more obs. -> higher science return Event driven commanding -command queue instead of timed commands -(Java)script instead of command executable -schedule execution can/will respond to events -scripts check and respond to telemetry -e.g. skip observation in case of errors, as failed peak-up or instrument anomaly -most efficient -flexible -scripts allow (quick) response to real-time events

12 12 Event driven commanding Each visit is composed of groups, sequences and activities -Some run sequential and some in parallel Visits can easily be removed or replaced

13 13 Lots of activities the coming years up to launch


Download ppt "1 Mission preparation Fred Lahuis SRON / Leiden Observatory MIRI NL Meeting ASTRON, 3 th June 2010."

Similar presentations


Ads by Google