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Power coupled between partially coherent vector fields in different states of coherence
1Cavendish Laboratory, University of Cambridge, Madingley Road, Cambridge, UK. stafford@mrao.cam.ac.uk
Summary
A new method calculates power coupled between partially coherent vector fields, crucial for submillimeter-wave astronomy optics. This technique simplifies power coupling calculations for optical design software.
Area of Science:
- Optics and Photonics
- Astronomy Instrumentation
- Electromagnetism
Background:
- Designing submillimeter-wave optical systems for astronomy requires accurate calculation of power coupling between optical fields.
- Partially coherent vector fields with varying coherence states present challenges in traditional optical design.
- Understanding coherence properties is vital for efficient signal transmission and detection in sensitive instruments.
Purpose of the Study:
- To develop a straightforward procedure for calculating power coupled between collimated, partially coherent vector fields.
- To provide a method applicable to fields in different states of coherence.
- To facilitate the integration of power coupling calculations into optical design software.
Main Methods:
- Introduced a method using coherence matrices of incoming (S) and outgoing (D) fields, denoted as A and B, respectively.
- Defined the power coupled (Ps) by the formula Ps = Tr(ATBT), where T represents the projection of basis functions.
- Extended the technique to calculate power coupling from background fields.
Main Results:
- A simplified formula, Ps = Tr(ATBT), was derived for calculating power coupled between partially coherent vector fields.
- The method was successfully illustrated by calculating power coupling between two scalar, Gaussian Schell-model beams.
- The procedure is general and can be applied to fields with different coherence properties.
Conclusions:
- The developed procedure offers an efficient and accurate way to calculate power coupling in optical systems.
- This method is particularly relevant for the design of submillimeter-wave astronomical instruments.
- The technique's compatibility with optical design software promotes its practical application in the field.