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| In preparation for beam studies on Mars. Mars will have a 8 arcsec diameter. The effective FWHM of gaussian beam observing it will differ from its nominal value as measured on a true point source according to the following curve: | Create on page per subject, but keep all update and new entry for the same subject in the same page otherwise discussions are too difficult to follow (e.g. below: subject Gaussian beam and Disk Planet, has 3 entries). - [[PlanetConvol |Gaussian beam and Disk Planet: May 29, 2012, NP; May 31, 2012, RZ; June 1st, 2012, NP]] - Prediction of field distortion from Zemax simulations, June 1, 2012, SL: [[attachment:NIKA_2012_grid_distortion.pdf]] |
Offline Processing Results
Create on page per subject, but keep all update and new entry for the same subject in the same page otherwise discussions are too difficult to follow (e.g. below: subject Gaussian beam and Disk Planet, has 3 entries).
- Gaussian beam and Disk Planet: May 29, 2012, NP; May 31, 2012, RZ; June 1st, 2012, NP
- Prediction of field distortion from Zemax simulations, June 1, 2012, SL: NIKA_2012_grid_distortion.pdf