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.
| Dune Field: ESP_063747_2450 ESP_063523_2450 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 64.50 | 315. | 23.6 | 6.414 | 64.0 | 61.8 |
| 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 |
| 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 |
| Pit in Hephaestus Fossae: ESP_063504_1995 ESP_055262_1995 (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 | 19.50 | 124. | 1.15 | -17.0 | 51.6 | 54.3 |
| 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 |
| 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 |
| Terrain Sample: ESP_063484_2205 ESP_063774_2205 (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 | 40.18 | 306. | 6.73 | 23.56 | 52.6 | 55.0 |
| Colorful Bedrock in a Northern Plains Crater: ESP_063376_2315 ESP_063956_2315 (Interval in Earth days: 45) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 51.00 | 14.5 | -1.5 | 26.06 | 54.8 | 61.3 |
| Iani Chaos: ESP_063206_1780 ESP_063852_1780 (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 | -2.13 | 343. | 3.24 | 27.44 | 55.5 | 54.1 |
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