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 Layer Tilts in Well-Exposed Layered Crater Floor Materials: ESP_055463_1485 ESP_059736_1485 (Interval in Earth days: 333) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -31.0 | 41.4 | 6.95 | -17.4 | 58.7 | 52.9 |
| Holden Crater Rim West of MSL Rover Landing Site: ESP_055268_1535 ESP_055413_1535 (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 | -26.3 | 324. | -1.9 | 17.99 | 59.3 | 56.6 |
| Crater Breach and Associated Channels : ESP_055266_2210 ESP_055411_2210 (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 | 40.88 | 10.8 | -3.3 | 11.29 | 59.3 | 60.3 |
| Candidate Landing Site for 2020 Mission near Jezero Crater : ESP_055567_1985 ESP_055501_1985 (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 | 18.17 | 76.9 | -1.5 | 16.73 | 55.3 | 53.2 |
| Lobate Landform near Reull Vallis : ESP_055250_1410 ESP_055527_1410 (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 | -38.5 | 97.0 | 5.92 | -10.2 | 64.5 | 62.3 |
| Crater East of Isidis Region : ESP_055263_1875 ESP_064204_1875 (Interval in Earth days: 697) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.428 | 96.2 | 6.56 | -24.0 | 51.4 | 58.9 |
| Deep Erosional Window into Niesten Crater Fill: ESP_055225_1520 ESP_055370_1520 (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 | -27.6 | 58.2 | 4.30 | 22.93 | 59.8 | 57.1 |
| Wrinkle Ridges in West Meridiani Planum : ESP_055201_1785 ESP_055346_1785 (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 | -1.46 | 349. | 6.45 | 25.83 | 52.0 | 50.3 |
| Meandering Channels on Western Edge of Acidalia Planitia : ESP_055519_2155 ESP_064038_2155 (Interval in Earth days: 664) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.34 | 304. | 0.23 | -20.2 | 60.3 | 61.3 |
| Thermokarst Channel Systems on Floor of Lyot Crater : ESP_055384_2310 ESP_055252_2310 (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 | 50.74 | 29.1 | -11. | 11.37 | 66.1 | 62.2 |
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