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- W1609623579 abstract "With few exceptions, measurements of cometary brightness and polarization have been restricted to regions in or near the coma and therefore to a relatively small range of phase angles. Photoelectric techniques are required for detailed wavelength coverage, whereas large-field photographic techniques are better suited for mapping the large regions of sky spanned by a comet tail. Observations with a small field of view provide high spatial resolution but generally restrict multicolor measurements of brightness and polarization to a small region of the comet. Observations with a large field of view (diameter larger than 1 or 2 deg) provide adequate color and spatial coverage but can result in the loss of detail. A compromise is afforded by Fabry photometry, using a modest telescope of small aperture and relatively large field of view." @default.
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- W1609623579 date "1976-01-01" @default.
- W1609623579 modified "2023-09-23" @default.
- W1609623579 title "Photoelectric Polarimetry of the Tail of Comet Ikey-Seki (1965 VIII)" @default.
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- W1609623579 doi "https://doi.org/10.1017/s0252921100500773" @default.
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