The Polarization of Supernova Light¶
Shapiro, P. R., & Sutherland, P. G. (1982). The Polarization of Supernova Light: A Measure of Deviation from Spherical Symmetry. The Astrophysical Journal.
Cited by¶
1 citation across 1 artifact.
Each citation links to the sentence it supports in the citing article.
Domain-specific¶
- Chandrasekhar Polarization
- Chandrasekhar's 1946 calculation predicted a rise from zero at disk center to about eleven percent at the limb for the ideal pure-scattering atmosphere. The classical exact conservative solution is conventionally quoted as a limiting local limb magnitude of approximately 11.713 percent.
This sourceThis independent vector-transfer application states the 11.7-percent conservative edge-on benchmark and develops the symmetry-to-net-polarization reasoning for unresolved scattering atmospheres.
- Chandrasekhar's 1946 calculation predicted a rise from zero at disk center to about eleven percent at the limb for the ideal pure-scattering atmosphere. The classical exact conservative solution is conventionally quoted as a limiting local limb magnitude of approximately 11.713 percent.
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Registry ID ref:a15f1d4471a8 · see in the full table