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.
| Layered Sinuous Ridge in the Argyre Planitia: ESP_012281_1240 ESP_012360_1240 (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 | -55.7 | 316. | -6.2 | 17.71 | 58.6 | 55.5 |
| Emission of Dark Material in Cerberus Fossae: ESP_011785_1875 ESP_011930_1875 (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 | 7.411 | 168. | -8.3 | 7.691 | 59.6 | 58.6 |
| Valleys along the Juventae Region Wallrock: ESP_011688_1760 ESP_019613_1760 (Interval in Earth days: 617) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.15 | 297. | 3.79 | -18.7 | 57.0 | 57.0 |
| Light-Toned Gully Material in Crater in Terra Sirenum: ESP_012380_1425 ESP_012802_1425 (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 | -37.4 | 130. | -7.3 | -22.4 | 52.4 | 47.4 |
| Compare Gullies in Crater to MOC Cproto For Change Detection: ESP_011727_1490 ESP_037704_1490 (Interval in Earth days: 2024) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -30.9 | 316. | 4.30 | -13.7 | 59.2 | 64.8 |
| Impact Crater Merged into Coprates Chasma: ESP_011767_1640 ESP_011833_1640 (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 | -15.9 | 302. | -3.0 | -24.0 | 57.3 | 58.6 |
| Landforms in the Tartarus Colles Region: ESP_012444_2065 ESP_014000_2065 (Interval in Earth days: 121) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.97 | 173. | 6.62 | -8.74 | 67.6 | 56.8 |
| Possible Pingos on Floor of Small Craters: ESP_011675_1470 ESP_015987_1470 (Interval in Earth days: 336) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -32.5 | 296. | -6.2 | -21.4 | 61.0 | 61.2 |
| Head of Rille East of Hecates Tholus: ESP_012036_2125 ESP_012748_2125 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.12 | 152. | 1.95 | 14.72 | 69.1 | 71.0 |
| Fans and Light-Toned Layers in Crater: ESP_012408_1465 ESP_030948_1465 (Interval in Earth days: 1444) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -33.2 | 84.2 | 8.09 | -3.93 | 50.4 | 37.5 |
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