Apr 7, 2023 · This work presented a case study connecting microscopic features to spectral characteristics for Venus' surface–atmosphere interactions.
Apr 2, 2023 · Understanding crust–atmosphere interactions on Venus is fundamentally important to interpretations of Venus' surface spectroscopic data.
The results showed that the oxidation of olivine produced magnesioferrite, magnetite, laihunite, hematite and maghemite at 470 degrees C and hematite, magnetite ...
The results showed that the oxidation of olivine produced magnesioferrite, magnetite, laihunite, hematite and maghemite at 470 °C and hematite, magnetite, ...
This work presented a case study connecting microscopic features to spectral characteristics for Venus' surface–atmosphere interactions. Further studies ...
High-Temperature Oxidation of Magnesium- and Iron-Rich Olivine under a CO 2 ... elevated temperature), could be used to trace olivine oxidation processes.
Missing: CO2 | Show results with:CO2
This work presented a case study connecting microscopic features to spectral characteristics for Venus' surface–atmosphere interactions. Further studies ...
The data in this experiment come from the high-temperature oxidation of olivine under CO2. In the experiment, olivine with different iron contents (Fa09, ...
Missing: Implications Venus.
High-Temperature Oxidation of Magnesium- and Iron-Rich Olivine under a CO2 Atmosphere: Implications for Venus. Remote Sens. 2023, 15, 1959. https://doi.org ...
High-Temperature Oxidation of Magnesium- and Iron-Rich Olivine under a CO2 Atmosphere: Implications for Venus by Zhong, Shan-Shan, Zhao, Yu-Yan Sara, Lin, ...