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.
| Well-Preserved 12 Kilometer Impact Crater on East Rim in Isidis Region: ESP_014016_1945 ESP_022376_1945 (Interval in Earth days: 652) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 14.52 | 98.4 | -8.6 | 14.23 | 48.5 | 51.5 |
| Gullies Observed by MOC: ESP_012707_1445 ESP_013208_1445 (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 | -35.4 | 201. | 2.07 | 23.84 | 46.6 | 38.4 |
| Possible Rootless Cones in Hydraotes Chaos: ESP_013177_1800 ESP_021458_1800 (Interval in Earth days: 645) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.053 | 326. | -4.9 | -21.2 | 49.8 | 53.9 |
| Dry Falls in the Southern Branch of Kasei Valles: ESP_013152_1980 ESP_013297_1980 (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 | 17.90 | 285. | 3.51 | 15.70 | 60.2 | 58.1 |
| Central Structure of a Large Impact Crater: ESP_013134_1610 ESP_021494_1610 (Interval in Earth days: 652) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.6 | 62.6 | -6.3 | 14.94 | 43.1 | 44.9 |
| Fractured Lava Dome in Eastern Tharsis Region: ESP_013904_1970 ESP_013970_1970 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 16.62 | 275. | -4.7 | -25.2 | 51.1 | 51.6 |
| Lineated Valley Fill in Nilosyrtis Mensae: ESP_012883_2135 ESP_013160_2135 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.01 | 68.2 | -3.0 | -23.7 | 72.4 | 72.3 |
| Gullied 35 Kilometer Diameter Impact Crater in Promethei Terra: ESP_013660_1475 ESP_013950_1475 (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 | -32.4 | 103. | 0.16 | 23.60 | 36.1 | 33.5 |
| Channel Cutting Wrinkle Ridge in Phlegra Dorsa: ESP_012985_2025 ESP_013130_2025 (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 | 22.00 | 164. | 4.41 | 19.35 | 64.2 | 62.2 |
| Volatiles and Gullies: ESP_013097_1115 ESP_013585_1115 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -68.4 | 1.31 | 2.13 | -13.5 | 53.0 | 53.2 |
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