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.
| Crater with Topographically Inverted Ejecta Blanket : ESP_052370_2485 ESP_052594_2485 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 68.15 | 231. | -7.1 | 8.166 | 51.0 | 49.1 |
| Crater in Baldet Crater : ESP_052284_2025 ESP_059959_2025 (Interval in Earth days: 598) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.41 | 66.1 | 8.05 | -11.8 | 38.6 | 37.7 |
| Twin Channels in Innsbruck Crater : ESP_052143_1735 ESP_052565_1735 (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 | -6.49 | 320. | -0.5 | -26.3 | 50.9 | 55.5 |
| Well-Preserved Crater North of Hellas Planitia : ESP_052218_1635 ESP_060183_1635 (Interval in Earth days: 620) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -16.1 | 74.3 | -6.3 | 5.878 | 58.1 | 48.6 |
| Possible Inverted Channel within Valley : ESP_052082_1680 ESP_052227_1680 (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 | -11.7 | 185. | 3.53 | 19.32 | 53.4 | 53.6 |
| Fan Material at an Alcove on Southwestern Aeolis Mons : ESP_052242_1745 ESP_063319_1745 (Interval in Earth days: 863) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.48 | 137. | -1.7 | 14.83 | 51.1 | 56.0 |
| Channel and Flow That Cut Crater Rim and Wall in Daedalia Planum : ESP_052357_1570 ESP_052568_1570 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -22.8 | 239. | 2.19 | -12.0 | 63.4 | 65.5 |
| Chains of Mounds in Utopia Planitia : ESP_052283_2075 ESP_052718_2075 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 27.04 | 94.1 | -5.7 | 21.52 | 39.1 | 37.7 |
| Light-Toned Mesa-Forming Materials in Terrain Cut by Samara Valles : ESP_052261_1570 ESP_035514_1570 (Interval in Earth days: 1305) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -22.6 | 341. | -9.5 | 4.984 | 63.1 | 68.5 |
| Candidate Red Dragon Landing Site in Arcadia Planitia : ESP_052358_2210 ESP_052134_2210 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.71 | 201. | 17.9 | -15.0 | 37.6 | 40.8 |
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