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 Cones in Aurorae Chaos: ESP_088540_1720 ESP_089107_1720 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.77 | 320. | 3.86 | -8.75 | 60.1 | 60.9 |
| Monitoring Gullied Crater: ESP_088568_2310 ESP_088634_2310 (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 | 50.71 | 266. | 8.41 | -6.17 | 44.4 | 45.9 |
| Gullies on Western Wall of Nier Crater: ESP_088574_2230 ESP_088640_2230 (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 | 42.77 | 105. | -0.5 | -17.0 | 44.0 | 45.8 |
| North Polar Layered Deposits Structural Geology in Icy Layers: ESP_088653_2625 ESP_088693_2625 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 82.34 | 81.4 | 8.18 | -8.30 | 58.5 | 59.6 |
| Channel Entering Sklodowska Crater: ESP_088512_2130 ESP_088578_2130 (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 | 32.92 | 358. | 15.6 | -3.74 | 42.6 | 44.5 |
| Fan-Shaped Feature in Ismenius Lacus: ESP_088485_2145 ESP_088696_2145 (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 | 33.95 | 17.5 | -4.9 | -15.7 | 44.2 | 45.9 |
| A Fissure and Channel near Pavonis Mons: ESP_086934_1775 ESP_087435_1775 (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 | -2.54 | 247. | -7.1 | 24.56 | 49.0 | 51.0 |
| Ring-Shaped Mounds in Ceraunius : ESP_086815_2115 ESP_087092_2115 (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 | 31.79 | 249. | 16.7 | -7.37 | 40.6 | 42.5 |
| Crater Infill: ESP_088354_1870 ESP_088565_1870 (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 | 6.953 | 356. | 10.0 | -5.16 | 51.1 | 52.6 |
| Planned ExoMars Landing Site in Oxia Planum: ESP_088157_1975 ESP_088447_1975 (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 | 17.33 | 336. | -8.6 | 8.83 | 47.5 | 46.8 |
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