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 Floor of Small Crater: ESP_012911_2165 ESP_013755_2165 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.13 | 23.1 | -0.1 | -21.7 | 74.4 | 68.5 |
| Mound on Nili Patera Floor: ESP_013582_1895 ESP_020940_1895 (Interval in Earth days: 574) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.139 | 67.3 | 1.63 | -17.6 | 49.9 | 58.9 |
| Eroded Layers in Northeast Gale Crater with Possible Sulfates: ESP_013263_1750 ESP_013685_1750 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.72 | 138. | 2.26 | -12.3 | 46.0 | 41.9 |
| 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 |
| Impact Crater with a Rocky Central Uplift: ESP_012947_1735 ESP_022441_1735 (Interval in Earth days: 740) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.55 | 125. | 4.88 | 27.14 | 48.6 | 37.0 |
| Rocky Deposit That Appears to Emanate from Warrego Valles Channel: ESP_012665_1365 ESP_012731_1365 (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 | -43.1 | 268. | 8.21 | -10.4 | 47.9 | 48.3 |
| Candidate Landing Site in Terra Sabaea and Tyrrhenna Terra Boundary: ESP_013925_1580 ESP_014426_1580 (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 | -21.7 | 66.6 | 0.50 | 25.72 | 34.3 | 32.1 |
| Putative Paleolake: ESP_013780_1630 ESP_058667_1630 (Interval in Earth days: 3497) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -16.7 | 64.7 | 1.57 | -15.2 | 35.8 | 31.8 |
| 3 Kilometer Diameter Crater on Edge of South Polar Layered Deposits: ESP_013344_0990 ESP_013463_0990 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -80.7 | 112. | -6.3 | -22.2 | 60.8 | 62.4 |
| Gullies in Dunes: ESP_014151_1325 ESP_021509_1325 (Interval in Earth days: 573) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -47.1 | 19.5 | 5.65 | -10.1 | 42.1 | 48.1 |
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