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- W3009027741 abstract "Abstract We present laboratory measurements of the phase functions and degree of linear polarization (DLP) curves of a selection of millimeter-sized cosmic dust analog particles. The set includes particles with similar sizes but diverse internal structure (compact and porous) and absorbing properties. The measured phase functions are found to be in all cases very different from those of micron-sized particles. They show a monotonic decrease with increasing phase angle from the back- to the side-scattering region, reaching a minimum at large phase angles before a steep increase of the forward peak. This is in stark contrast to the phase functions of micron-sized particles, which are rather flat at low and intermediate phase angles. The maximum of the DLP for millimeter-sized compact particles is shifted toward larger phase angles (∼130°) compared to that of micron-sized particles (∼90°). Porosity plays an important role in the measured DLP curves: the maximum significantly decreases for increasing porosity as a result of multiple scattering within the particle. Large porous particles with highly absorbing inclusions can reproduce both the OSIRIS/ Rosetta phase functions and ground-based DLP observations of comet 67P/Churyumov–Gerasimenko." @default.
- W3009027741 created "2020-03-06" @default.
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- W3009027741 date "2020-02-24" @default.
- W3009027741 modified "2023-10-17" @default.
- W3009027741 title "Experimental Phase Function and Degree of Linear Polarization Curves of Millimeter-sized Cosmic Dust Analogs" @default.
- W3009027741 cites W1901401340 @default.
- W3009027741 cites W1982916468 @default.
- W3009027741 cites W1983832799 @default.
- W3009027741 cites W1987500393 @default.
- W3009027741 cites W1995816972 @default.
- W3009027741 cites W2001956405 @default.
- W3009027741 cites W2007620586 @default.
- W3009027741 cites W2008874157 @default.
- W3009027741 cites W2009827313 @default.
- W3009027741 cites W2011270334 @default.
- W3009027741 cites W2018533264 @default.
- W3009027741 cites W2034159489 @default.
- W3009027741 cites W2034388546 @default.
- W3009027741 cites W2035089871 @default.
- W3009027741 cites W2041607647 @default.
- W3009027741 cites W2042112467 @default.
- W3009027741 cites W2049824100 @default.
- W3009027741 cites W2050505309 @default.
- W3009027741 cites W2059280245 @default.
- W3009027741 cites W2062714504 @default.
- W3009027741 cites W2064917563 @default.
- W3009027741 cites W2076985067 @default.
- W3009027741 cites W2080426384 @default.
- W3009027741 cites W2092598616 @default.
- W3009027741 cites W2115755906 @default.
- W3009027741 cites W2121855215 @default.
- W3009027741 cites W2128761389 @default.
- W3009027741 cites W2136564862 @default.
- W3009027741 cites W2137345295 @default.
- W3009027741 cites W2140190919 @default.
- W3009027741 cites W2156771656 @default.
- W3009027741 cites W2164235908 @default.
- W3009027741 cites W2192239197 @default.
- W3009027741 cites W2254961145 @default.
- W3009027741 cites W2255533209 @default.
- W3009027741 cites W2270111979 @default.
- W3009027741 cites W2328359704 @default.
- W3009027741 cites W2473308294 @default.
- W3009027741 cites W2520198316 @default.
- W3009027741 cites W2520649120 @default.
- W3009027741 cites W2580930080 @default.
- W3009027741 cites W2588514328 @default.
- W3009027741 cites W2593241750 @default.
- W3009027741 cites W2601451320 @default.
- W3009027741 cites W2621644291 @default.
- W3009027741 cites W2736899547 @default.
- W3009027741 cites W2737509499 @default.
- W3009027741 cites W2740074169 @default.
- W3009027741 cites W2744608329 @default.
- W3009027741 cites W2758847266 @default.
- W3009027741 cites W2766101201 @default.
- W3009027741 cites W2768603813 @default.
- W3009027741 cites W2771360123 @default.
- W3009027741 cites W2773547565 @default.
- W3009027741 cites W2790829749 @default.
- W3009027741 cites W2900053734 @default.
- W3009027741 cites W2909710102 @default.
- W3009027741 cites W2942849753 @default.
- W3009027741 cites W2953811967 @default.
- W3009027741 cites W2964622611 @default.
- W3009027741 cites W3098336062 @default.
- W3009027741 cites W3100493054 @default.
- W3009027741 cites W3100606073 @default.
- W3009027741 cites W3101846756 @default.
- W3009027741 cites W3102748656 @default.
- W3009027741 cites W3104855411 @default.
- W3009027741 cites W3106472861 @default.
- W3009027741 cites W3122955073 @default.