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GRID CALIBRATION OVERVIEW

GOAL:

bullet Knowledge to ~1% of grid pair transmission, modulation amplitude and phase,

as a function of energy and source offset,

expressed in a manner that can be efficiently applied to the data.


MOTIVATION:

bulletArtifact-free light-curves
bullet
bulletHigh dynamic range imaging
bulletUnbiased and artifact-free spectroscopy


METHOD:

  1. Obtain optical, x-ray, mass and thickness calibration data on individual grids
  2. Define a tractable grid model consistent with calibration data
  3. Calculate single grid transmission, spatial modulation and phase (E, angle)
  4. Combine single grid results to get grid pair transmission, modulation amplitude and phase.
  5. (Sub-collimator response table)

  6. Integrate and interpolate sub-collimator response table as necessary for individual flares.
  7. (Grid response matrix)

  8. Use in-flight self-calibration to refine grid models as needed.

 

 

PRIMARY OBSERVATIONAL DATA

bulletOPTICAL MEASUREMENTS OF GRID SURFACE
bulletAverage pitch
bulletAverage rms deviation
bulletSlat width distribution (+unknown constant)
bulletAverage slit orientation
bulletPosition of slits (phase)
bulletX-RAY
bulletPeak transmission for Cd109, Co57, Cs137 (23, 122, 662 kev)
bulletFWHM of single grid transmission at 23 and 122 kev
bullet1-degree transmission at 122 and 662 kev
bulletMISCELLANEOUS
bulletMass of stacked grid (Tecomet)
bulletGrid thickness at rims (Tecomet)
bulletDimensions and mass of typical spare blades (VBC)

 

WEAKNESSES IN OBSERVATIONAL DATA

 

bulletNo direct measurements of slit widths of individual layers (Tecomet)
bulletNo direct measurement of surface density of unetched Tecomet grid layers
bulletNo direct measurements of average profile of stacked slit edges
bulletNo direct measurements of tilt distribution for VBC blades

 

 

 

STATUS OF GRID CALIBRATION TASK

bulletOptical data fully analyzed
bulletUsed as basis for grid alignment
bulletAlignment independently confirmed by gridlet test
bulletDetermination of grid model parameters is in progress
bulletVBC grid data self-consistent to 1 – 2%
bulletTecomet grid parameters consistent to ~5%
bulletSoftware to convert grid parameters to sub-collimator response table is working
bulletSome additional features are being added
bulletSoftware to apply grid calibration data for imaging and spectroscopy is in SSW.

 

SELF-CALIBRATION

GOAL

bulletUse internal redundancy to fine-tune grid parameters.

 

FEATURES

bulletApproach: Adjust grid parameters until corrected count rate ratios are independent of (low) energy and flare location
bulletHigh energy response is not sensitive to details of grid model.
bulletUses count rates, rather than modulation (much more sensitive)
bulletRecalculated sub-collimator response table should be stable and common to all flares
bulletNot a user-task.
bulletProcedures to be verified before launch using simulated data.

EXAMPLES OF TECHNIQUE

bulletGrid phase determined by elimination of ‘wobble’ in single sub-collimator image
bulletTilt is corrected by elimination of 4-second periodicity in corrected light curves
bulletSlit/thickness ratio is determined by elimination of 2-second periodicity in corrected count rates.
bulletEffective slit width is determined by comparing peak Tecomet and VBC grid count rate ratios

 

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Responsible NASA Official:  Gordon D. Holman

Web Design:  Merrick Berg, Brian Dennis, Gordon Holman, & Gilbert Prevost

Heliophysics Science Division
NASA/Goddard Space Flight Center
Laboratory for Solar Physics/ Code 671
Greenbelt, MD, 20771, USA
Gordon.D.Holman@nasa.gov

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This site last updated November 10, 2008.