File:11214 2023 956 Fig3 HTML.webp
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Summary
| Description |
English: "Venus looks bland in nearly all the visible wavelengths—but other wavelengths reveal myriad details. From left to right: dayside false color image from Akatsuki’s UVI instrument (PLANET-C Project); dayside false color image from Akatsuki’s UVI and IR1 instruments (PLANET-C Project); composite of dayside imagery from MESSENGER that shows natural color (NASA/JHUAPL/CIW/ Gordon Ugarkovic); nightside image from PSP centered on Ovda Regio (Wood et al. 2022); nightside image of the same area from Akatsuki’s IR1 instrument, but rotated (PLANET-C Project); nightside synthesized false color image from Akatsuki’s IR2 instrument (PLANET-C Project); stack of five pseudo-color infrared images from Akatsuki’s LIR instrument (PLANET-C Project); microwave observations from the Very Large Array (Butler et al. 2001); and a surface 3D model derived from Magellan radar imagery (NASA Visualization Technology Applications and Development). Images at shorter wavelengths are made using sunlight reflected from the dayside of Venus. Longer-wavelength images record thermal emission from the surface and/or atmosphere. Finally, the radar images show the power of active sounding to reveal surface features"[1] |
| Date | |
| Source | https://link.springer.com/article/10.1007/s11214-023-00956-0/figures/3 |
| Author | O’Rourke, J.G., Wilson, C.F., Borrelli, M.E. et al. |
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- ↑ O’Rourke, Joseph G. (2023). "Venus, the Planet: Introduction to the Evolution of Earth’s Sister Planet". Space Science Reviews 219 (1). Springer Science and Business Media LLC. DOI:10.1007/s11214-023-00956-0. ISSN 0038-6308.
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
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| current | 21:57, 6 July 2023 | | 1,434 × 932 (99 KB) | Nsae Comp | Uploaded a work by O’Rourke, J.G., Wilson, C.F., Borrelli, M.E. et al. from https://link.springer.com/article/10.1007/s11214-023-00956-0/figures/10 with UploadWizard |
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