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- W3173463113 abstract "Three-color observations of the nightglow brightness and polarization were made at the Majaky Observatory in October 1969 to determine the brightness of zodiacal light at the ecliptic pole. On the assumption that the degree of polarization of zodiacal light is 0.20 at the ecliptic pole, the corresponding brightnesses are found to be 68, 70, and 96 G2 stars of the 10th magnitude per square deg. at 0.37, 0.53, and 0.58μ. The large diurnal variations in observed intensity and direction of polarization are attributed to the effects of dust in the Earth’s atmosphere." @default.
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- W3173463113 date "1971-06-01" @default.
- W3173463113 modified "2023-09-23" @default.
- W3173463113 title "On the Influence of the Atmospheric Dust on the Zodiacal Light Polarization" @default.
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- W3173463113 doi "https://doi.org/10.1017/s0252921100049162" @default.
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