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.
| Landslide Alcove Within the Arsia Mons Southwest Rift Zone: PSP_009910_1690 PSP_010543_1690 (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 | -10.7 | 239. | 17.3 | -3.84 | 60.3 | 60.4 |
| Multiple Unconformities in the Upper North Polar Layered Deposits: PSP_010181_2600 PSP_010234_2600 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.74 | 23.4 | -6.9 | -18.7 | 64.6 | 66.2 |
| Possible Intravalley Paleolake in Shalbatana Vallis: PSP_009683_1830 PSP_010316_1830 (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 | 2.989 | 316. | -5.0 | -21.7 | 54.6 | 56.7 |
| Alcove with Bright Rocky Slope Streaks: PSP_009762_1905 PSP_009907_1905 (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 | 10.40 | 318. | -0.3 | 15.26 | 51.2 | 50.3 |
| Central Uplift of Hargraves Crater in the Nili Fossae Region: PSP_009639_2010 PSP_010272_2010 (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 | 20.73 | 75.8 | -5.4 | -21.0 | 47.8 | 52.1 |
| Interaction of Cratered Cone and Crater Ejecta: PSP_009906_2225 PSP_010196_2225 (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 | 42.33 | 343. | -7.7 | 14.62 | 48.0 | 48.7 |
| Hydrated Light-Toned Layers on Crater Floor: PSP_010274_2140 PSP_010696_2140 (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 | 33.63 | 17.0 | 5.05 | -8.32 | 49.3 | 54.8 |
| Possible Pingos in Gusev Crater: PSP_009385_1655 PSP_009886_1655 (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 | -14.2 | 175. | -18. | 5.226 | 65.1 | 63.0 |
| Well-Preserved Crater with Central Peak: PSP_009367_1590 ESP_035357_1590 (Interval in Earth days: 2025) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -20.6 | 306. | -5.0 | 9.569 | 68.4 | 66.5 |
| Junction of Three Polar Troughs: PSP_010030_2670 PSP_010532_2670 (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 | 86.74 | 162. | -8.8 | -21.4 | 67.2 | 74.3 |
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