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- W1661527217 abstract "We develop a physical model of the zodiacal cloud incorporating the real dust sources of asteroidal, cometary, and kuiperoidal origin. Using the inferred distribution of the zodiacal dust, we compute its thermal emission and scattering at several wavelengths (1.25, 5, and 20 $mu$m) as a function of NGST location assumed to be at 1 AU or 3 AU. Areas on the sky with a minimum of zodiacal light are determined." @default.
- W1661527217 created "2016-06-24" @default.
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- W1661527217 date "1999-10-29" @default.
- W1661527217 modified "2023-09-27" @default.
- W1661527217 title "The NGST and the zodiacal light in the Solar system" @default.
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