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.
| Pitted Material and Mounds in Chryse Planitia: ESP_063536_2210 ESP_055294_2210 (Interval in Earth days: 642) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.42 | 326. | 6.38 | -6.29 | 53.4 | 59.8 |
| Gullies Incising Mantle-Filled Alcove in Western Argyre Region: ESP_063748_1330 ESP_037401_1330 (Interval in Earth days: 2053) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -46.4 | 309. | 14.1 | -7.46 | 74.4 | 74.7 |
| Ares Vallis Deposit: ESP_063483_1875 ESP_086324_1875 (Interval in Earth days: 1779) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.559 | 338. | 3.40 | 19.63 | 53.0 | 38.4 |
| Possible Deltas in Crater in Amazonis Planitia: ESP_063462_1985 ESP_063752_1985 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.27 | 190. | 8.53 | 29.19 | 50.7 | 51.0 |
| Candidate ExoMars Landing Site in Oxia Planum: ESP_063760_1990 ESP_063826_1990 (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 | 18.63 | 335. | -3.2 | -23.6 | 54.1 | 56.6 |
| Cones in Cydonia Colles: ESP_063799_2190 ESP_055491_2190 (Interval in Earth days: 647) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 38.6 | 346. | 2.96 | 15.13 | 56.8 | 60.2 |
| Amazonis Planitia: ESP_063422_2185 ESP_063488_2185 (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 | 38.35 | 199. | 8.91 | -8.72 | 51.2 | 53.6 |
| Flow-Like Feature within the Adamas Labyrinthus: ESP_063452_2195 ESP_063887_2195 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.12 | 100. | 3.32 | 28.83 | 52.2 | 55.8 |
| Steep Slopes and Dunes in East Coprates Chasma: ESP_063524_1650 ESP_063458_1650 (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 | -14.6 | 302. | 0.84 | 24.26 | 60.7 | 59.1 |
| Medusae Fossae Formation above Athabasca Valles Lavas: ESP_063780_1840 ESP_063925_1840 (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 | 3.899 | 150. | -4.4 | 9.655 | 55.5 | 54.9 |
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