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.
| Candidate Future Landing Site: ESP_034808_1655 ESP_034874_1655 (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 | -14.3 | 175. | 1.98 | -21.3 | 60.1 | 62.0 |
| Gully Without Apron: ESP_034628_2340 ESP_035063_2340 (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 | 53.73 | 41.1 | -2.0 | 18.22 | 45.1 | 42.5 |
| Dune Change Detection in Juventae Chasma: ESP_034843_1775 ESP_035054_1775 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.58 | 298. | 2.91 | -7.48 | 53.0 | 54.8 |
| Fan and Channel Forms in Memnonia Sulci Region: ESP_034768_1695 ESP_035757_1695 (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 | -10.5 | 186. | 6.76 | -7.65 | 57.1 | 61.5 |
| Contact of Medusae Fossae Formation with Flank of Apollinaris Mons: ESP_034597_1730 ESP_034663_1730 (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 | -6.92 | 174. | 12.3 | -12.5 | 53.2 | 55.4 |
| Lava Flow North of Ascraeus Mons: ESP_034739_1975 ESP_035240_1975 (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 | 17.37 | 255. | -1.0 | 16.11 | 43.6 | 44.0 |
| Light-Toned Stratified Materials in Eastern Candor Chasma: ESP_034896_1725 ESP_036452_1725 (Interval in Earth days: 121) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.55 | 292. | -3.8 | 11.60 | 56.7 | 58.2 |
| Ejecta Flow over and around Pre-Existing Obstacles: ESP_034690_2175 ESP_035336_2175 (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 | 37.19 | 150. | 7.52 | 28.85 | 40.3 | 39.0 |
| Layered Rocks of Ophir Mensa: ESP_034738_1760 ESP_034949_1760 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.81 | 285. | -3.5 | -14.7 | 53.5 | 55.5 |
| Domoni Crater Secondaries: ESP_034845_2305 ESP_035280_2305 (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 | 50.02 | 236. | -1.8 | 22.27 | 43.3 | 41.1 |
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