Published June 15, 2015
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Analytical Modelling of Thirty Meter Telescope Optics Polarization
Chicago
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Abstract
The polarization introduced due to Thirty Meter Telescope (TMT) optics is calculated using an analytical model. Mueller matrices are also generated for each optical element using Zemax, based on which the instrumental polarization due to the entire system at the focal plane is estimated and compared with the analytical model. This study is significant in the estimation of the telescope sensitivity and also has great implications for future instruments.
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© 2015 SPIE.Attached Files
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Additional details
- Eprint ID
- 61057
- Resolver ID
- CaltechAUTHORS:20151013-123129467
- Created
-
2015-10-13Created from EPrint's datestamp field
- Updated
-
2021-11-10Created from EPrint's last_modified field
- Series Name
- Proceedings of SPIE
- Series Volume or Issue Number
- 9654