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Q Band OOF results from Jan 8, 2008

Note: for contemporaneous Mustang results, goto this page

Q Band results (with Zernikes enabled) from TPAR_18 (Todd)

Because these scans were taken in 'AzEl' mode rather than 'Encoder' mode, I had to compute azoff and eloff in post-processing. This included calculating precession from J2000 to the current epoch, annual aberration, and applying the refraction correction from the Antenna file. The diurnal aberration term was ignored as it is <= 0.3 arcsec. The resulting scan pattern is very nearly centered at (0,0). The buildoof2008.py script (attached below) will perform these corrections whenever it encounters data recorded in AzEl? mode. The fits on this page include up to 5th order Zernikes, to be consistent with the corresponding Mustang plots.

-- ToddHunter - 01 Feb 2008

Attachment: sort Action: Size: Date: Who: Comment:
obsbeam-1.png action 9246 01 Feb 2008 - 20:27 ToddHunter  
obsbeam-2.png action 7681 01 Feb 2008 - 20:29 ToddHunter  
obsbeam-3.png action 9687 01 Feb 2008 - 20:29 ToddHunter  
bestfitbeams-0.png action 6035 01 Feb 2008 - 20:33 ToddHunter  
bestfitbeams-1.png action 5481 01 Feb 2008 - 20:33 ToddHunter  
bestfitbeams-2.png action 6075 01 Feb 2008 - 20:33 ToddHunter  
aperture-phase.png action 14708 01 Feb 2008 - 20:33 ToddHunter  
buildoof2008.py action 17471 01 Feb 2008 - 20:35 ToddHunter invocation: buildoof2008.qbuild20080108()
session.py action 11274 01 Feb 2008 - 20:36 ToddHunter precession, aberration calcs added for AzEl? mode
s39-l-db.fits action 192960 01 Feb 2008 - 20:38 ToddHunter debaselined FITS file
oof2.png action 43645 04 Feb 2008 - 21:24 ToddHunter comparison of 7mm and 3mm phase maps

Topic 2008Jan08QBandOOFResults . { Edit | Attach | Ref-By | Printable | Diffs | r1.4 | > | r1.3 | > | r1.2 | More }
Revision r1.4 - 12 Feb 2008 - 15:50 GMT - ToddHunter
Parents: WebHome > InformationForProjectTeam > AntennaCharacterizationSpring2005 > OOFHolography > OOFWithMustang2008Jan23Meeting > 2008Jan08MustangOOFResults
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