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.
| West of Erebus Montes : ESP_055220_2185 ESP_090048_2185 (Interval in Earth days: 2713) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 38.23 | 186. | 0 | -21.8 | 57.4 | 57.1 |
| Junctions between Wide Channels and Narrow Channels : ESP_055538_1735 ESP_063358_1735 (Interval in Earth days: 609) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.67 | 151. | -2.0 | 24.76 | 53.0 | 55.7 |
| Linear Vent Structure East of Olympus Mons : ESP_055403_1975 ESP_059676_1975 (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 | 17.36 | 233. | 6.12 | -17.6 | 53.2 | 36.9 |
| Terrace-Based Well-Preserved Pitted Material of Crater in Kasei Valles : ESP_055440_2105 ESP_063247_2105 (Interval in Earth days: 608) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 30.38 | 302. | -5.1 | -25.4 | 57.9 | 51.6 |
| Gully Comparison on Northern and Southern Rims of Asimov Crater : ESP_055570_1330 ESP_064247_1330 (Interval in Earth days: 676) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -46.6 | 4.45 | -8.2 | 25.99 | 65.1 | 67.5 |
| Cross-Bedding in Layers on Steep Scarp : ESP_055357_1540 ESP_059986_1540 (Interval in Earth days: 361) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -25.9 | 54.3 | 7.71 | -2.15 | 57.8 | 52.5 |
| 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 |
| Wrinkle Ridge in Solis Planum : ESP_055283_1580 ESP_073483_1580 (Interval in Earth days: 1418) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.4 | 274. | 3.78 | -18.8 | 57.0 | 59.0 |
| Sinuous Ridges North of Gale Crater : ESP_055578_1760 ESP_059996_1760 (Interval in Earth days: 344) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.89 | 137. | 20.6 | 8.802 | 50.9 | 39.6 |
| Korolev Crater Layers : ESP_055260_2530 ESP_055247_2530 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 72.91 | 163. | 7.20 | -8.16 | 74.6 | 75.5 |
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