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.
Fractures and Uplifted Portion of Floor of Echus Chasma: ESP_021908_1810 ESP_021842_1810 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.856 | 279. | -17. | 4.9 | 50.1 | 49.2 |
Victoria Crater: ESP_021747_1780 ESP_022380_1780 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.04 | 354. | -2.8 | -23.0 | 49.2 | 43.5 |
Potential Mars Landing Site near Mounds Associated with Crater Rim: ESP_021919_2135 ESP_021642_2135 (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 | 32.97 | 336. | -23. | -0.04 | 71.4 | 71.0 |
Ridges around Crater Rim Valley in Terra Cimmeria: ESP_021901_1395 ESP_021756_1395 (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 | -40.3 | 113. | 9.90 | -3.69 | 39.8 | 42.6 |
Impact Crater with Central Uplift: ESP_021998_1610 ESP_022420_1610 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.8 | 344. | -5.5 | -20.5 | 40.2 | 36.6 |
Many Small Cones in Amazonis Planitia: ESP_021990_1985 ESP_022412_1990 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.78 | 198. | -4.5 | -18.4 | 59.5 | 56.0 |
Central Uplift with Layers and Clays: ESP_021688_1325 ESP_021754_1325 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -47.2 | 170. | 2.61 | -14.9 | 44.6 | 45.1 |
Hematite in Eos Chasma: ESP_021775_1665 ESP_022408_1665 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.3 | 311. | -3.6 | -23.2 | 44.4 | 38.4 |
Kaiser Crater Dune Gullies: ESP_021720_1330 ESP_020876_1330 (Interval in Earth days: 65) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -46.7 | 20.1 | -22. | 3.645 | 46.0 | 56.9 |
Lava Flow Features in Marte Vallis: ESP_021964_2015 ESP_030232_2015 (Interval in Earth days: 645) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.01 | 186. | 4.43 | -13.0 | 60.8 | 64.2 |
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