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.
| Intriguing Dark Dunes in Proctor Crater: PSP_003101_1320 ESP_011909_1320 (Interval in Earth days: 686) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -47.7 | 30.6 | 22.7 | -2.86 | 58.7 | 61.9 |
| Slope Streaks in Terra Sabaea South of Janssen Crater: PSP_003694_1800 ESP_030409_1800 (Interval in Earth days: 2081) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.082 | 37.9 | -4.8 | -27.3 | 54.3 | 53.4 |
| Small Scallops Suggesting Sublimation O North Bank of Auqakuh Vallis: PSP_003482_2115 PSP_005895_2115 (Interval in Earth days: 188) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 31.05 | 60.7 | 6.34 | 26.06 | 68.8 | 48.6 |
| Potential Currently-Active Gullies in Fresh Crater: PSP_003939_1420 ESP_012549_1420 (Interval in Earth days: 671) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.6 | 192. | 7.82 | 27.83 | 44.6 | 47.0 |
| Channel Flow: PSP_003978_1715 PSP_004334_1715 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.28 | 205. | -3.3 | 7.629 | 48.8 | 44.2 |
| Light-Toned Deposit in Tithonium Chasma: PSP_003514_1755 PSP_005848_1755 (Interval in Earth days: 182) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.60 | 271. | 6.07 | -6.81 | 52.9 | 34.2 |
| Cerberus Fossae and Diverse Morphologies: PSP_003241_1880 PSP_003531_1880 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.700 | 164. | -6.5 | 25.78 | 58.2 | 55.6 |
| Light Toned Ridges in Meridiani Region: PSP_003682_1805 PSP_003972_1805 (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 | 0.329 | 5.15 | -0.2 | 29.79 | 54.2 | 50.0 |
| Exposure of South Polar Layered Deposit: PSP_003341_0935 PSP_003406_0935 (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 | -86.4 | 9.61 | -0.0 | 16.50 | 75.3 | 72.7 |
| Comparative Gully Morphology: PSP_003557_1335 PSP_004058_1335 (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 | -46.1 | 183. | 1.07 | 19.97 | 52.5 | 43.7 |
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