Comparison of remote sensing observations of planetary wind streaks
Autor: | Shimrit Maman, Dan G. Blumberg, Aviv Lee Cohen-Zada |
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Rok vydání: | 2019 |
Předmět: |
010504 meteorology & atmospheric sciences
biology 0208 environmental biotechnology Streak Soil Science Geology Venus 02 engineering and technology Mars Exploration Program biology.organism_classification 01 natural sciences 020801 environmental engineering law.invention symbols.namesake law Radar imaging symbols Aeolian processes Terrestrial planet Computers in Earth Sciences Radar Titan (rocket family) 0105 earth and related environmental sciences Remote sensing |
Zdroj: | Remote Sensing of Environment. 232:111342 |
ISSN: | 0034-4257 |
DOI: | 10.1016/j.rse.2019.111342 |
Popis: | Wind streaks are common aeolian features observed on terrestrial planets. They were first identified on Mars; thus, the associated terminology is based on Mars-related observations usually describing surface patterns with distinct albedos. However, terms related to reflected tones are only relevant to past knowledge for Mars, and not necessarily suitable for description of radar-visible streaks located on Venus, Titan, or Earth. Furthermore, the sensor type used to observe wind streaks can influence the subsequent data analysis. The purpose of this study was to examine the effects of sensor type on wind streak identification and interpretation. Six case studies featuring wind streaks on Earth were performed, using imaging by both radar and optical sensors. The results indicate that wind streak identification is constrained to a specific combination of sensor settings appropriate for the local surface properties. Only half the optically visible wind streaks considered in this study were also radar-visible, but all the wind streaks observable in the radar images also appeared in the optical images. Furthermore, “bright” and “dark” (reflectance and backscatter) are relative terms and should be used with caution. These results suggest that the Venusian wind streak database is most likely far from complete and that many more streaks exist. |
Databáze: | OpenAIRE |
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