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.
Viscous Flow in Protonilus Mensae: ESP_017024_2230 ESP_017314_2230 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 42.61 | 55.3 | -10. | 8.248 | 42.7 | 40.9 |
Eastern Portion of Well-Preserved 10-Kilometer Diameter Impact Crater: ESP_017101_1810 ESP_017312_1810 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.766 | 116. | 7.04 | -2.87 | 50.2 | 52.0 |
Coprates Chasma Wall: ESP_017200_1680 ESP_017912_1680 (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 | -11.7 | 296. | -9.0 | 1.653 | 59.3 | 61.1 |
Layered Mesa in Candor Chasma: ESP_017266_1715 ESP_017411_1715 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.17 | 294. | -9.6 | 5.488 | 57.5 | 57.2 |
Exposure of Lower Layers in South Melas Chasma with Stratigraphic Contacts: ESP_016963_1680 ESP_018598_1680 (Interval in Earth days: 127) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.1 | 286. | -0.9 | 16.30 | 57.5 | 60.1 |
Fracture in Orcus Patera: ESP_017191_1935 ESP_026896_1935 (Interval in Earth days: 756) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 13.24 | 178. | 0 | 13.59 | 45.3 | 45.7 |
Possible Olivine-Rich Terrain: ESP_016903_1820 ESP_018248_1820 (Interval in Earth days: 105) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 1.941 | 123. | 0.64 | -15.9 | 48.8 | 54.5 |
Filled Crater in Amazonis Planitia at End of Marte Vallis: ESP_017032_2050 ESP_018100_2050 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.66 | 198. | -5.6 | 7.91 | 42.0 | 43.4 |
Tempe Terra Fault Scarp: ESP_017002_2270 ESP_017134_2270 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 46.88 | 293. | 4.81 | -23.9 | 42.5 | 44.7 |
Possible Phyllosilicates in Davies Crater: ESP_016960_2265 ESP_017949_2265 (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 | 45.96 | 0.18 | 5.68 | -8.98 | 42.3 | 43.7 |
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