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.
| Lava Flow Spilling over Crater Wall onto Crater Floor in Daedalia Planum: ESP_026354_1480 ESP_035281_1480 (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 | -31.8 | 222. | -5.4 | 15.66 | 73.9 | 74.0 |
| Well-Exposed Bedrock Layers in Northern Hellas Planitia: ESP_026492_1540 ESP_036052_1540 (Interval in Earth days: 745) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -25.9 | 54.4 | -4.8 | 7.826 | 70.0 | 70.5 |
| Cratered Cones with Divergent Wakes Near Grjota Valles: ESP_026369_1965 ESP_028413_1965 (Interval in Earth days: 159) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 16.52 | 167. | -8.3 | 7.177 | 44.8 | 50.8 |
| Northern Plains Craters: ESP_026446_2305 ESP_027158_2305 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 50.09 | 219. | 0 | 16.82 | 42.3 | 43.0 |
| Complex Superposition of Fractures: ESP_026286_2235 ESP_026563_2235 (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 | 43.31 | 269. | -3.0 | -21.3 | 41.0 | 43.0 |
| Possible Future Mars Landing Site of 2018 Joint Rover: ESP_026270_1820 ESP_027747_1820 (Interval in Earth days: 115) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.165 | 350. | 3.38 | -8.58 | 50.3 | 53.3 |
| Bedform Changes Southwest of Schiaparelli Crater: ESP_026322_1720 ESP_027166_1720 (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 | -7.72 | 13.0 | -3.6 | -18.2 | 56.9 | 59.2 |
| Fresh Crater: ESP_026365_2260 ESP_027710_2260 (Interval in Earth days: 105) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 45.42 | 271. | 1.37 | 20.86 | 41.0 | 45.7 |
| Central Peaks of an Impact Crater: ESP_026243_2200 ESP_053697_2200 (Interval in Earth days: 2139) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.83 | 4.05 | -5.5 | 8.701 | 40.8 | 41.3 |
| Basin in Northeast Hellas Region: ESP_026412_1525 ESP_026557_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 | -27.2 | 78.2 | 0 | 15.95 | 70.4 | 69.9 |
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