Table 1
Information of datasets used in this study.
| Martian day | LS (°) | LTST | SZA (°) | Inc. (ROIs) (°) | Emi. (ROIs) (°) | Pha. (ROIs) (°) |
|---|---|---|---|---|---|---|
| Sol 05 | 47.0 | 11:02–11:19 | 12–15 | 13–24 | 66–85 | 59–90 |
| Sol 32 | 59.3 | 16:22–16:39 | 60–63 | 60–66 | 65–77 | 3–124 |
| Sol 58 | 71.0 | 16:41–16:59 | 63–67 | 64–71 | 66–84 | 3–125 |
| Sol 84 | 82.5 | 09:12–09:29 | 34–38 | 32–37 | 47–78 | 15–110 |
| Sol 99 | 89.5 | 16:41–16:59 | 63–66 | 65–69 | 64–81 | 32–125 |
Notes. LS, LTST, and SZA refer to the solar longitude, local true solar time, and solar zenith angle during the acquisition of the panoramic images. Inc., Emi., and Pha. (ROIs) denote the ranges of incidence, emission, and phase angles for the regions of interest (ROIs) used for phase curve extraction. These angles were topographically corrected using the digital elevation model.
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