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.
| Possible Repetitive Bedding in Eastern Medusae Fossae Formation : ESP_050960_1835 ESP_051105_1835 (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 | 3.559 | 216. | -3.8 | 11.32 | 35.8 | 35.8 |
| Contact in Western Hellas Planitia : ESP_050979_1415 ESP_051124_1415 (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 | -37.9 | 63.2 | -6.8 | 5.638 | 58.0 | 59.6 |
| Meroe Patera Dune Monitoring : ESP_051084_1875 ESP_050939_1875 (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 | 7.174 | 67.7 | 25.4 | 12.24 | 33.7 | 33.9 |
| Layered Light-Toned Deposits on Floor of Orson Welles Crater : ESP_050996_1790 ESP_051919_1790 (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 | -1.19 | 313. | -4.7 | 10.12 | 37.3 | 45.3 |
| Channel and Fan Structure of Ceraunius Tholus : ESP_050945_2050 ESP_051235_2050 (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 | 24.69 | 262. | 2.86 | 27.57 | 37.0 | 34.5 |
| Debris Apron-Like Textures in Nereidum Montes : ESP_050548_1395 ESP_050614_1395 (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 | -40.0 | 310. | -3.8 | -22.6 | 52.2 | 54.4 |
| Inverted Features and Layers in Dia-Cau Crater: ESP_050864_1795 ESP_052354_1795 (Interval in Earth days: 116) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.40 | 317. | 1.11 | 14.53 | 35.5 | 47.8 |
| Well-Preserved Impact Crater : ESP_050625_2160 ESP_050915_2160 (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 | 35.84 | 357. | 4.38 | 23.26 | 44.4 | 40.6 |
| Mound in Utopia Planitia : ESP_050529_2095 ESP_055144_2095 (Interval in Earth days: 360) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 29.33 | 99.8 | 2.02 | 25.24 | 41.5 | 51.4 |
| Eastern Floor of Roddy Crater: ESP_050508_1580 ESP_050086_1580 (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 | -21.7 | 320. | -12. | 15.28 | 40.5 | 33.2 |
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