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.
| Landforms in Centauri Montes Region : ESP_028706_1410 ESP_028772_1410 (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 | -38.5 | 95.7 | 4.18 | -15.4 | 67.0 | 67.7 |
| Crater in Utopia Planitia : ESP_028719_2290 ESP_037646_2290 (Interval in Earth days: 695) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 48.46 | 89.3 | 0 | -13.9 | 61.7 | 65.9 |
| Pettit Crater Ejecta in Contact with Knobs and Massifs : ESP_028887_1900 ESP_042245_1900 (Interval in Earth days: 1041) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.773 | 188. | -5.0 | -18.3 | 54.6 | 39.9 |
| Distal Rampart of Toconao Crater : ESP_028699_1585 ESP_028844_1585 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.4 | 285. | -6.4 | 7.649 | 60.3 | 58.3 |
| Well-Preserved Impact Crater : ESP_028830_2040 ESP_042043_2040 (Interval in Earth days: 1030) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.59 | 303. | -5.3 | -28.5 | 55.9 | 42.2 |
| Possible Inverted Stream Channels Near Mariner Crater : ESP_028887_1430 ESP_055431_1430 (Interval in Earth days: 2068) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.6 | 193. | 3.30 | 24.96 | 64.1 | 60.0 |
| Distorted Icy Terrain in Nilosyrtis Mensae Crater : ESP_028601_2145 ESP_028324_2145 (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 | 34.17 | 73.6 | -1.8 | 13.89 | 55.3 | 50.7 |
| Possible Repetitive Bedding Near Base of Central Lobe of Medusae Fossae : ESP_028650_1695 ESP_028795_1695 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -10.4 | 180. | 8.61 | 21.62 | 55.7 | 54.2 |
| Layering in Graben Wall : ESP_028793_2265 ESP_072482_2265 (Interval in Earth days: 3404) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 45.91 | 229. | 0 | 24.14 | 61.8 | 55.9 |
| IR-Distinct Crater : ESP_028676_2185 ESP_054152_2185 (Interval in Earth days: 1986) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 38.06 | 185. | -2.3 | -20.3 | 57.5 | 46.8 |
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