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.
| Extra-Crater Sinuous Ridge: ESP_083174_1035 ESP_083161_1035 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -76.1 | 320. | 7.79 | -7.99 | 61.6 | 62.9 |
| Rim of Osuga Valles: ESP_083134_1635 ESP_083200_1635 (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 | -16.2 | 320. | 8.94 | -14.6 | 49.7 | 50.7 |
| Juventae Chasma Interior Deposit Layers: ESP_082937_1760 ESP_082357_1760 (Interval in Earth days: 45) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.16 | 297. | 8.05 | -7.44 | 54.7 | 58.4 |
| Scour Pit Island in Southeastern Part of Medusae Fossae Formation: ESP_083046_1795 ESP_083191_1795 (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 | -0.69 | 201. | -0.6 | 13.40 | 55.9 | 53.9 |
| Inflated Lava Flows in Southern Tharsis Region: ESP_083137_1585 ESP_083203_1585 (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 | -21.1 | 239. | 6.66 | -16.7 | 49.0 | 49.9 |
| Sub-Kilometer Well-Preserved Impact Crater with Extensive Secondaries: ESP_083265_1460 ESP_083476_1460 (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 | -33.4 | 347. | -4.6 | -3.58 | 47.4 | 44.5 |
| Noachis Terra Channels: ESP_083106_1560 ESP_083172_1560 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -23.9 | 6.27 | 2.56 | -19.9 | 49.3 | 50.2 |
| Terrain Sample in Aeolis Planum: ESP_082969_1810 ESP_083892_1810 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.792 | 143. | 5.12 | -5.74 | 56.4 | 49.0 |
| Mantling Unit in Tithonium Chasma: ESP_083083_1750 ESP_083149_1750 (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 | -4.70 | 271. | 4.04 | -20.1 | 53.8 | 55.1 |
| Crater: ESP_083271_1585 ESP_083772_1585 (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 | -21.2 | 181. | 0 | 13.72 | 47.8 | 40.5 |
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