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.
Possible Arete in North and South Debris Flows: ESP_013528_1380 ESP_013673_1380 (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 | -41.6 | 108. | -4.1 | 9.479 | 39.1 | 37.6 |
Fretted Terrain-Like Aprons Near Reull Vallis: ESP_013001_1415 ESP_013146_1415 (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 | -38.4 | 97.3 | -15. | -1.78 | 44.3 | 41.5 |
Stratigraphy of Possible Sulfate and Zeolite at Mawrth Vallis: ESP_013229_2050 ESP_013295_2050 (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 | 24.51 | 341. | 14.8 | -5.47 | 63.5 | 64.0 |
Lineated Valley Fill in Nilosyrtis Mensae: ESP_014162_2135 ESP_020597_2135 (Interval in Earth days: 501) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.08 | 68.5 | 6.58 | -16.0 | 59.0 | 66.6 |
Unusual Dune Form along Inner Small Crater Rim: ESP_013909_1145 ESP_014041_1145 (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 | -65.1 | 151. | -0.4 | -20.7 | 51.9 | 54.5 |
Possible Rootless Cones in Acidalia Planitia: ESP_013559_2195 ESP_022473_2195 (Interval in Earth days: 694) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.31 | 331. | 0.73 | -25.2 | 72.1 | 71.4 |
Excellent Exposure of Layered Mound in Terby Crater: ESP_013872_1520 ESP_014017_1520 (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 | -27.5 | 74.3 | 1.04 | 15.03 | 34.6 | 33.2 |
Bright Gully Deposits in Western Hale Crater: ESP_013230_1445 ESP_014074_1445 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.0 | 322. | 8.51 | -20.1 | 39.3 | 37.8 |
Basal Exposure of South Polar Layered Deposits: ESP_013145_1070 ESP_013277_1070 (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 | -73.0 | 133. | 0.46 | -14.5 | 55.6 | 56.1 |
Steep Lobate Scarps in Kasei Valles: ESP_012717_1910 ESP_013139_1910 (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 | 10.88 | 282. | 2.07 | -8.93 | 59.1 | 56.6 |
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