The spectropolarimetry of planets. I - The observation procedure and the data reduction method

Details The spectropolarimetry of planets. I - The observation procedure and the data reduction method The spectropolarimetry of planets. I - The observation procedure and the data reduction method

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986kfnt....2...41g&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 2, May-June 1986, p. 41-47. In Russian.

Astronomy and Astrophysics

Astronomy

1

Astronomical Spectroscopy, Planetology, Polarimetry, Solar System, Algorithms, Data Reduction, Gas Giant Planets, Moon, Terrestrial Planets

Scientific paper

The observation of Jupiter, Saturn, Mars, Venus, the moon, and Vega by
means of a spectropolarimeter equipped with a 127-deg achromatic
waveplate is discussed. The spectropolarimeter characteristics are
described, and the data reduction algorithm is presented.

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