S
S. L. Odell
Researcher at University of California, Berkeley
Publications - 7
Citations - 413
S. L. Odell is an academic researcher from University of California, Berkeley. The author has contributed to research in topics: Synchrotron radiation & Polarization (waves). The author has an hindex of 7, co-authored 7 publications receiving 405 citations.
Papers
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Journal ArticleDOI
Transfer of polarized radiation in self-absorbed synchrotron sources. I. Results for a homogeneous source
T. W. Jones,S. L. Odell +1 more
TL;DR: In this paper, the solution to the equation of transfer of polarized radiation in a steady-state homogeneous rarefied medium is applied to self-absorbed synchrotron sources.
Journal ArticleDOI
Transfer of polarized radiation in self-absorbed synchrotron sources. II - Treatment of inhomogeneous media and calculation of emergent polarization
T. W. Jones,S. L. Odell +1 more
TL;DR: In this paper, a transfer procedure based on the coupled-wave formulation was derived, which allows consideration of inhomogeneous sources, and it was shown that plasma characteristic wave eccentricities in a source must be fairly large unless Faraday rotation per absorption depth is very large.
Journal ArticleDOI
The changes in spectral-flux distribution during variability of extragalactic nonthermal sources, 0.36 to 3.5 microns.
TL;DR: In this article, the spectral-flux distributions of variable extragalactic sources have been observed over the wavelength range 0.36 µm to 3.5 µm in terms of injection and energy loss of high-energy electrons radiating synchrotron radiation.
Journal ArticleDOI
Radio emission from bright, optically selected quasars
Journal ArticleDOI
Coordinated photometric and spectroscopic observations of strong extragalactic 90 GHz sources
S. L. Odell,J. J. Puschell,W. A. Stein,F. N. Owen,R. W. Porcas,S. L. Mufson,T. J. Moffett,M. H. Ulrich +7 more
TL;DR: In this paper, nearly simultaneous radio and infrared-optical observations were obtained for several extragalactic radio sources which are strong at 90 GHz, showing that the spectral-flux distributions are generally peaked or flat over the radio portion of the spectrum with a steeper, power-law behavior at infraredoptical frequencies.