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Coherence, power laws, and the negative polarization surge
Gorden Videen1, Karri Muinonen, Kari Lumme
1U.S. Army Research Laboratory, AMSRL-CI-EE, 2800 Powder Mill Road, Adelphi, Maryland 20783-1197, USA. gvideen@arl.army.mil
Applied Optics
|July 2, 2003
Summary
This study introduces a new ray-tracing model to explain negative polarization in astronomical bodies. The model, based on path length distribution, accurately reproduces observed wavelength-independent polarization.
Area of Science:
- Astronomy and Astrophysics
- Radiative Transfer
- Polarimetry
Background:
- Astronomical bodies often exhibit negative polarization, a phenomenon not fully explained by existing models.
- Understanding polarization is crucial for characterizing celestial object composition and structure.
Purpose of the Study:
- To develop a novel second-order ray-tracing model to account for negative polarization in astronomical bodies.
- To investigate the role of constructive interference and Fresnel reflections in generating negative polarization.
Main Methods:
- Developed a second-order ray-tracing model incorporating constructive interference of reciprocal rays.
- Utilized Fresnel reflections from an inverse gamma-type distribution function of path length.
- Modeled ray paths incident upon astronomical bodies.
Main Results:
- The model successfully predicts the negative polarization branch observed in some astronomical bodies.
- The predicted negative polarization is largely independent of wavelength.
- Polarization magnitude is primarily determined by the power law in the path-length distribution.
Conclusions:
- The developed ray-tracing model provides a viable explanation for negative polarization in astronomical objects.
- The findings align with observational data, particularly the wavelength independence of the polarization.
- Path-length distribution is a key factor in determining the observed polarization characteristics.