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.
| Meanders and Tributaries in Ridge Form in the Zephyria Region: ESP_024484_1750 ESP_024985_1750 (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 | -5.09 | 151. | 4.43 | 19.16 | 38.5 | 43.0 |
| Lava Coating, Flood-Carved Kasei Valles: ESP_024202_2010 ESP_024703_2010 (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 | 20.84 | 287. | -2.9 | 19.15 | 38.0 | 35.7 |
| The Eastern Floor of Aram Chaos: ESP_024266_1830 ESP_023910_1830 (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 | 3.112 | 340. | 24.6 | 9.188 | 33.0 | 32.9 |
| Crater Rim with Possible Columnar Jointing: ESP_024288_1945 ESP_024710_1945 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 14.52 | 98.3 | 21.7 | 6.703 | 34.1 | 36.4 |
| Possible Future Landing Site at Edge of Libya Montes: ESP_024038_1835 ESP_023405_1835 (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 | 3.516 | 86 | 5.65 | 27.23 | 33.6 | 32.4 |
| MSL Rover Landing Site in Gale Crater: ESP_024234_1755 ESP_024300_1755 (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 | -4.64 | 137. | -5.2 | -24.4 | 36.6 | 38.8 |
| Possible Bedform Changes in Medusae Fossae: ESP_024047_1895 ESP_024113_1895 (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 | 9.508 | 197. | 25.0 | 5.939 | 32.7 | 34.4 |
| Valleys on Western Hecates Tholus: ESP_024207_2130 ESP_024352_2130 (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 | 32.52 | 149. | -0.4 | 16.28 | 43.3 | 41.0 |
| MSL Landing Site in Gale Crater: ESP_023957_1755 ESP_024023_1755 (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 | -4.55 | 137. | 15.1 | -6.86 | 32.6 | 34.9 |
| Dunes: ESP_024060_1205 ESP_023928_1205 (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 | -59.1 | 218. | -18. | 5.39 | 67.4 | 63.9 |
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