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.
| Intercrater Terrain in Terra Sabaea : ESP_043292_1550 ESP_044413_1550 (Interval in Earth days: 88) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.6 | 44.9 | 7.30 | -23.9 | 63.3 | 69.4 |
| Small Fan in Crater West of Mangala Valles : ESP_043418_1640 ESP_043563_1640 (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 | -15.6 | 204. | -3.2 | 14.43 | 58.6 | 58.5 |
| Wrinkle Ridge Near Ganges Catena : ESP_043217_1770 ESP_042716_1770 (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 | -3.08 | 290. | 2.42 | -19.3 | 49.2 | 46.8 |
| Meanders in Ridge Form in the Zephyria Region : ESP_024695_1745 ESP_025407_1745 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.40 | 151. | -7.4 | 9.959 | 41.9 | 48.3 |
| Marching Dust Devils: ESP_042201_1715 ESP_043190_1715 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.26 | 310. | -2.6 | -28.5 | 42.9 | 54.2 |
| Steep Slopes in Melas Chasma: ESP_043072_1685 ESP_043573_1685 (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 | -11.3 | 290. | -7.9 | 19.28 | 53.5 | 55.3 |
| Double-Terrace Crater in Arcadia Planitia: ESP_043036_2275 ESP_043102_2275 (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 | 47.23 | 183. | 16.5 | 2.794 | 42.2 | 43.0 |
| Chaotic Terrain in Xanthe Terra: ESP_042926_1780 ESP_059673_1780 (Interval in Earth days: 1305) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.04 | 315. | -2.3 | 8.467 | 46.8 | 35.4 |
| Central Melas Chasma Floor: ESP_042927_1680 ESP_045749_1680 (Interval in Earth days: 220) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.7 | 288. | -0.0 | 20.23 | 51.9 | 53.9 |
| Possible Sulfate-Rich Terrain in Northeast Syrtis Major Region: ESP_042750_1970 ESP_043172_1970 (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 | 16.63 | 77.4 | 7.00 | -9.18 | 39.0 | 41.7 |
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