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.
| Pits Fissures and Channels East of Olympus Mons : ESP_044841_1960 ESP_044907_1960 (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 | 15.86 | 233. | 6.54 | -11.9 | 43.6 | 45.1 |
| Multiple Yardang Units and Directions in Memnonia Sulci : ESP_044777_1725 ESP_086343_1725 (Interval in Earth days: 3239) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.48 | 184. | -7.6 | -17.1 | 56.3 | 45.6 |
| Wrinkle Ridge and Channel Intersection along Huygens Crater Rim : ESP_044729_1600 ESP_045006_1600 (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 | -19.8 | 56.3 | -1.0 | -15.5 | 64.2 | 64.1 |
| Possible Phyllosilicates in Knobs within Depression on Dichotomy Boundary : ESP_044995_2165 ESP_052023_2165 (Interval in Earth days: 548) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.32 | 347. | 7.00 | 27.66 | 41.0 | 36.1 |
| Candidate Hardpan in Loire Valles : ESP_044969_1590 ESP_052208_1590 (Interval in Earth days: 564) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -20.6 | 345. | -5.6 | 21.96 | 64.2 | 59.4 |
| Cerberus Fossae : ESP_044672_1875 ESP_045305_1875 (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 | 7.205 | 169. | -8.3 | 7.712 | 48.4 | 46.9 |
| Unusual Structures in North Polar Layered Deposits : ESP_044794_2620 ESP_045308_2620 (Interval in Earth days: 40) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 81.91 | 60.4 | -8.8 | 5.241 | 59.7 | 63.2 |
| Fractured Surface Near Athabasca Valles Lava : ESP_044831_1825 ESP_053560_1825 (Interval in Earth days: 680) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.431 | 148. | 3.35 | 17.54 | 49.8 | 49.5 |
| Mamers Valles Source : ESP_044915_2205 ESP_044770_2205 (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 | 40.34 | 12.2 | -7.8 | -23.2 | 42.3 | 43.2 |
| North Polar Layered Deposits 160-Meter Diameter Crater Monitoring : ESP_044810_2620 ESP_044784_2620 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 81.84 | 333. | 7.95 | -6.74 | 59.0 | 59.6 |
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