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.
| Partly-Filled Impact Crater near Nicholson Crater: ESP_082176_1830 ESP_082242_1830 (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 | 2.848 | 196. | -7.6 | -23.2 | 59.3 | 60.7 |
| Clusters of Craters and Landform near Hephaestus Fossae: ESP_082271_2050 ESP_090591_2050 (Interval in Earth days: 649) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.76 | 121. | -6.6 | 7.281 | 64.8 | 58.1 |
| Proposed Site for Future Exploration in Coprates Chasma: ESP_082304_1645 ESP_082238_1645 (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 | -15.3 | 305. | -5.3 | 10.96 | 58.1 | 57.2 |
| Two-Toned Bedrock Exposed in 5-Kilometer Crater in Noachis Terra: ESP_082144_1480 ESP_082078_1480 (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 | -31.8 | 354. | -8.4 | 7.7 | 62.4 | 61.9 |
| Terrain Sample: ESP_082313_1660 ESP_082524_1660 (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 | -13.7 | 59.6 | -5.7 | -23.6 | 58.0 | 58.2 |
| Lava-Coated Crater near Kasei Valles: ESP_082265_1960 ESP_082555_1960 (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 | 15.66 | 285. | 1.99 | 21.45 | 61.3 | 61.1 |
| Channels Inside Perrotin Crater: ESP_082252_1775 ESP_082542_1775 (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 | -2.34 | 282. | 4.78 | 27.61 | 57.8 | 55.3 |
| A Song of Ice and Tectonics: ESP_081922_1470 ESP_081856_1470 (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 | -32.6 | 294. | -4.2 | 13.49 | 64.7 | 64.1 |
| Channels in Hebrus Valles: ESP_082073_2025 ESP_082429_2025 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.32 | 125. | -4.3 | 21.18 | 62.2 | 62.9 |
| Site Dubbed Bilbao: ESP_081902_0930 ESP_081903_0930 (Interval in Earth days: 0) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.0 | 127. | 29.2 | 14.38 | 87.8 | 89.1 |
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