Instrument Performance Requirements

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Presentation transcript:

Instrument Performance Requirements HMI00374 Instrument Performance Requirements Jesper Schou Instrument Scientist jschou@solar.stanford.edu

Instrument Performance Req. – Overview Observing Scheme Derivations of Subsystem Requirements Instrument Performance Document IPD Development Schedule

Observing Scheme Observables Dopplergrams Magnetograms, vector and line-of-sight Others: Intensity, line depth, etc. Observables made from filtergrams described by framelists Filtergram properties Wavelength Polarization state Exposure time Camera ID Compression parameters, … Determined by subsystem settings E.g. motor positions Framelists List of filtergrams repeated at fixed cadence during normal operations Entirely specified in software – Highly flexible

Framelist Example Time: Time of first exposure at given wavelength since start of framelist execution Tuning: I1, I2, … specify the tuning position Doppler pol.: Polarization of image taken with Doppler camera L and R indicate left and right circular polarization Vector pol.: Polarization of image taken with vector camera 1, 2, 3, 4: Mixed polarizations needed to make vector magnetograms

Instrument Performance Document Purpose Capture derivations of filtergram and subsystem requirements Use for testing/calibration/characterization Capture actual performance Contents HMI overview Instrument overview Summary of science requirements Observables to filtergram flow Details of derivations Summary of derived requirements Filtergram to subsystem flow Summary of requirements for each subsystem As measured performance Observable Requirements Filtergram Requirements Subsystem Requirements

Summary of Filtergram Requirements

Summary of Subsystem Requirements

IPD Development Schedule Draft IPD provided with Concept Study Report Improved draft available at PDR Complete version by CDR Continued evolution throughout mission As measured performance