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.
| Nili Patera Dunes: ESP_040021_1890 ESP_040654_1890 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.998 | 66.9 | -4.2 | -21.4 | 50.3 | 43.8 |
| Crater on South Polar Layered Deposits: ESP_040070_0960 ESP_040110_0960 (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 | -83.7 | 194. | 8.19 | -7.80 | 63.1 | 64.5 |
| Valleys in Crater in Noachis Terra: ESP_039931_1555 ESP_040788_1555 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.0 | 8.50 | -4.8 | 21.63 | 37.9 | 32.5 |
| Pasted-on Material on Crater Ejecta: ESP_040131_1930 ESP_040487_1930 (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 | 13.00 | 302. | 3.43 | 15.22 | 51.1 | 45.8 |
| Candidate Landing Site for 2020 Mission in Hadriacus Palus: ESP_040113_1525 ESP_040390_1525 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.0 | 78.4 | 8.57 | -18.6 | 35.1 | 35.9 |
| Region North of Samara Valles: ESP_039998_1620 ESP_040987_1620 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -17.5 | 338. | -4.3 | -19.4 | 38.3 | 35.5 |
| Gullies and Lobate Material on Massif in Nereidum Montes: ESP_040131_1405 ESP_049559_1405 (Interval in Earth days: 735) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.1 | 309. | 0.39 | 20.00 | 37.4 | 35.7 |
| Slopes of Layered Deposits: ESP_040078_1715 ESP_048372_1715 (Interval in Earth days: 646) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.43 | 313. | -11. | 13.46 | 40.9 | 41.3 |
| Crater with Light-Toned Wall Rock in Outflow Channel Floor: ESP_040038_1760 ESP_041238_1760 (Interval in Earth days: 93) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.97 | 324. | -5.5 | -20.6 | 42.9 | 36.0 |
| Daedalia Planum Lava Flow: ESP_039910_1470 ESP_040543_1470 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -32.8 | 222. | 5.35 | -14.7 | 37.2 | 36.8 |
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