In addition to planned stereo pairs, the Pairendipity software can identify all overlapping images suitable for stereo processing. Global lists of such image pairs for the HiRISE and CTX datasets are provided here ordered by latitude. Images taken close together in time minimize illumination and frost differences and are especially useful (see the Delta-Days column). Stereo images planned within the same 14-day operations cycle are known as SPORCs.
Crater Ejecta Lower Than Plains: ESP_018709_2290 ESP_019197_2290 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 48.73 | 127. | 13.4 | -11.4 | 46.3 | 53.4 |
Layered Terrain in Aeolis Planum: ESP_018603_1755 ESP_019592_1755 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.68 | 150. | 5.39 | -11.1 | 56.5 | 56.6 |
Gemina Lingula Scarp with Outcrop of Layered Deposits and Unconformities: ESP_018778_2605 ESP_018897_2605 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.23 | 26.7 | 6.03 | -9.11 | 61.6 | 63.8 |
Well-Preserved Impact Crater: ESP_018758_2420 ESP_026538_2420 (Interval in Earth days: 606) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 61.71 | 229. | -2.3 | -19.3 | 52.4 | 48.1 |
Crosscutting Relationships between Persbo Crater Ejecta and Viscous Flows: ESP_018550_1890 ESP_019262_1890 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.989 | 156. | -8.3 | 4.302 | 50.9 | 51.2 |
Milankovic Crater: ESP_018785_2345 ESP_019220_2345 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 54.20 | 212. | 5.45 | 25.97 | 49.2 | 52.3 |
Lava Channel on the North Flank of Ascraeus Mons: ESP_018520_1920 ESP_018665_1920 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.95 | 254. | -4.6 | 13.12 | 49.3 | 48.3 |
Pit with Channels Southeast of Tooting Crater: ESP_018759_2025 ESP_019260_2025 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.10 | 208. | -2.8 | 14.99 | 47.0 | 48.2 |
Layered Ejecta of Lonar Crater: ESP_018501_2540 ESP_018554_2540 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 73.67 | 39.3 | 1.88 | -18.0 | 55.7 | 57.6 |
Noctis Labyrinthus: ESP_018533_1730 ESP_019522_1730 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.81 | 260. | 12.7 | -4.27 | 57.3 | 56.8 |
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