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.
| Ridges or Flows in Northeast Gale Crater: ESP_025790_1750 ESP_027135_1750 (Interval in Earth days: 104) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.71 | 137. | -6.0 | 3.949 | 52.2 | 55.9 |
| Small Mounds in Chryse Planitia: ESP_025427_1995 ESP_025282_1995 (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 | 19.37 | 322. | 6.11 | -10.3 | 39.2 | 40.0 |
| Mantle Layers in Crater in Terra Cimmeria: ESP_025474_1380 ESP_051847_1380 (Interval in Earth days: 2055) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -41.6 | 127. | 4.28 | -18.6 | 74.1 | 73.7 |
| Well-Preserved Impact Crater in Utopia Planitia: ESP_025514_2045 ESP_025870_2045 (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 | 24.44 | 107. | 0.69 | 16.37 | 39.3 | 39.0 |
| Clusters of Buttes and Mesas among Flows South of Western Cerberus Fossae: ESP_025684_1885 ESP_026040_1880 (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 | 7.775 | 149. | -6.7 | 6.019 | 45.2 | 46.2 |
| Well Preserved 7-Kilometer Impact Crater in Utopia Planitia: ESP_025791_1945 ESP_025646_1945 (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 | 14.46 | 104. | 24.6 | 6.969 | 40.6 | 41.4 |
| Wrinkle Ridge Superimposed on Well-Preserved Crater: ESP_025468_1640 ESP_024835_1640 (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 | -15.7 | 288. | -5.8 | 12.96 | 56.2 | 47.5 |
| Finely Stratified Units in Northeast of Gale Crater: ESP_025724_1755 ESP_025579_1755 (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 | -4.54 | 137. | 5.03 | -14.8 | 50.9 | 51.1 |
| Flow Draped over Crater Rim Visible in CTX Image : ESP_025563_1975 ESP_025207_1975 (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 | 17.48 | 209. | 15.2 | 2.131 | 39.4 | 38.8 |
| Contact between Yardang-Forming Material and Platy Flow Material: ESP_025473_1840 ESP_034255_1840 (Interval in Earth days: 684) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.897 | 149. | -3.9 | 28.53 | 45.2 | 43.3 |
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