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.
| Layers in Trough Floor and Scarp of Western Bench of Terby Crater: ESP_016206_1525 ESP_016351_1525 (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 | -27.4 | 74.5 | 8.70 | 23.26 | 59.0 | 59.9 |
| Bedrock Exposed by Impact Crater: ESP_016275_1535 ESP_016420_1535 (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 | -26.1 | 350. | 8.04 | 23.11 | 59.0 | 59.8 |
| Crater Rim Gullies Filled with Small Dunes: ESP_015934_2165 ESP_037243_2165 (Interval in Earth days: 1660) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.09 | 292. | 1.58 | -16.4 | 42.8 | 56.6 |
| Athabasca Valles: ESP_016071_1890 ESP_024708_1890 (Interval in Earth days: 673) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.934 | 155. | 7.83 | -16.8 | 39.6 | 38.8 |
| Crescentic Scour Features in Mff: ESP_016254_1830 ESP_016399_1830 (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 | 2.753 | 201. | -8.2 | 8.768 | 44.1 | 44.0 |
| Possible MSL Landing Site in Holden Crater: ESP_015999_1535 ESP_016276_1535 (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 | -26.4 | 325. | 13.9 | -13.6 | 55.0 | 60.5 |
| Bedrock Exposures in Wall of Impact Crater: ESP_016152_2115 ESP_017075_2115 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 31.01 | 102. | -1.6 | 10.61 | 40.8 | 40.0 |
| Stranded Lobe of Material with Associated Ridge on Valley Floor: ESP_016238_2180 ESP_017161_2180 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.54 | 273. | -3.4 | 6.789 | 42.5 | 40.5 |
| Massif in Deuteronilus Mensae: ESP_016141_2260 ESP_016431_2260 (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 | 45.44 | 39.7 | 3.75 | 23.76 | 45.5 | 42.2 |
| Fresh Impact Crater in Northern Plains: ESP_016164_2170 ESP_016797_2170 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.79 | 133. | 4.17 | -6.96 | 41.9 | 41.7 |
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