Planned stereo pairs have suitable stereo convergence angles and illumination by design.
In addition to planned stereo pairs, the Pairendipity software can identify overlapping
HiRISE images that are serendipitously suitable for stereo processing and find stereo
pairs within the CTX dataset.
Planned HiRISE stereo pairs are listed in the “Stereo Pair List (CSV)” link below.
Since this list is based on produced stereo anaglyphs it also contains a few serendipitous
pairs that underwent special processing. Most serendipitous HiRISE stereo pairs are listed
in the “Pairendipity Stereo” link, while CTX stereo pairs are listed
in “Pairendipity CTX Stereo”.
Images taken close together in time minimize illumination and frost differences and are
especially useful (see the Delta-Days column in the Pairendipity files or difference
the orbit numbers in the image IDs in the Stereo Pair List file). Stereo pairs
with both images planned within the same 14-day (168-orbit) operations cycle are known as SPORCs.
| South Polar Layered Deposits Exposed in Promethei Lingula: ESP_013714_0970 ESP_013687_0970 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -82.8 | 116. | -28. | -8.52 | 66.4 | 64.2 |
| Gullies: ESP_012722_1400 ESP_012867_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 | -39.6 | 153. | -6.2 | 7.111 | 47.5 | 44.4 |
| Ejecta Flow from Bacolor Crater: ESP_014147_2135 ESP_022494_2135 (Interval in Earth days: 651) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.32 | 118. | -1.3 | -27.5 | 59.9 | 66.5 |
| Bedrock Exposures in Uzboi Vallis and a Crater Rim: ESP_013586_1490 ESP_021722_1490 (Interval in Earth days: 634) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -30.8 | 323. | -0.0 | -28.7 | 36.4 | 44.3 |
| Gullies: ESP_013130_1350 ESP_013631_1350 (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 | -44.5 | 174. | 0.49 | 17.76 | 42.6 | 38.0 |
| Light-Toned Outcrops along Ius Region Wallrock: ESP_012849_1705 ESP_013126_1705 (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 | -9.22 | 281. | -3.9 | -28.8 | 49.2 | 48.0 |
| Central Uplift of an Impact Crater in Hesperia Planum: ESP_013211_1675 ESP_013633_1675 (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 | -12.4 | 118. | 8.88 | -5.92 | 42.9 | 39.0 |
| 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 |
| Central Peak of Large Well-Preserved Crater: ESP_013198_1660 ESP_021545_1660 (Interval in Earth days: 651) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.7 | 113. | 8.48 | -27.9 | 42.6 | 48.8 |
| Lava Flow Margin in Echus Chasma: ESP_013271_1810 ESP_013693_1810 (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 | 1.211 | 279. | 2.08 | -12.7 | 48.9 | 44.8 |
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