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.
Small Delta or Fan: ESP_082191_1735 ESP_082257_1735 (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 | -6.65 | 147. | 7.15 | -9.95 | 57.5 | 58.7 |
Topographic Interactions in Athabasca Valles: ESP_082217_1895 ESP_082283_1895 (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 | 9.431 | 156. | -1.6 | -17.5 | 59.9 | 61.4 |
Two-Toned Bedrock Exposed in 5-Kilometer Crater in Noachis Terra: ESP_082144_1480 ESP_082078_1480 (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 | -31.8 | 354. | -8.4 | 7.7 | 62.4 | 61.9 |
Hematite-Rich Terrain in West Candor Chasma: ESP_082120_1745 ESP_082331_1745 (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 | -5.24 | 285. | -1.4 | 12.00 | 58.3 | 56.8 |
Spiders with Large Spring Fans: ESP_082112_0970 ESP_082113_0970 (Interval in Earth days: 0) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -82.8 | 167. | 4.86 | -29.9 | 83.5 | 86.8 |
Light-Toned Mesas near Mawrth Vallis: ESP_082395_2040 ESP_074074_2040 (Interval in Earth days: 648) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.60 | 336. | -0.5 | -23.0 | 65.0 | 68.7 |
Hillslope Morphologies in Rim of Vinogradov Crater: ESP_082211_1615 ESP_082277_1615 (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 | -18.1 | 323. | 5.12 | -11.5 | 58.1 | 58.9 |
Chryse Chaos: ESP_082290_1885 ESP_082356_1885 (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 | 8.575 | 323. | 8.00 | -7.61 | 59.2 | 60.6 |
Banded Terrain and Layering in Hellas Planitia: ESP_082221_1400 ESP_082366_1400 (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 | -39.9 | 53.0 | 6.65 | 29.05 | 62.6 | 58.7 |
Terrain Sample: ESP_082131_1830 ESP_082408_1830 (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 | 2.782 | 343. | 9.02 | -2.09 | 57.9 | 59.0 |
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