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.
| Spiders : ESP_055605_0930 ESP_055604_0930 (Interval in Earth days: 0) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -86.8 | 170. | 7.43 | 23.09 | 86.4 | 85.0 |
| Bright and Dark Seasonal Fans : ESP_055945_0945 ESP_055944_0945 (Interval in Earth days: 0) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -85.4 | 252. | -7.3 | 17.64 | 80.3 | 78.2 |
| Gully Monitoring : ESP_055642_1430 ESP_055497_1430 (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 | -36.4 | 193. | 26.5 | 8.779 | 57.1 | 60.4 |
| Spiders with Big Spring Fans : ESP_055947_0970 ESP_055948_0970 (Interval in Earth days: 0) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -82.6 | 167. | 9.03 | -28.5 | 77.0 | 80.4 |
| Spider Terrain : ESP_055981_0870 ESP_055982_0870 (Interval in Earth days: 0) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -86.8 | 86.2 | 8.96 | 25.98 | 82.2 | 81.5 |
| Terrain Dubbed Inca City Monitoring : ESP_055639_0985 ESP_055692_0985 (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 | -81.3 | 295. | 4.23 | -8.55 | 82.4 | 82.4 |
| Candidate Landing Site for 2020 Mission near Jezero Crater : ESP_055567_1985 ESP_055501_1985 (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 | 18.17 | 76.9 | -1.5 | 16.73 | 55.3 | 53.2 |
| Thermokarst Channel Systems on Floor of Lyot Crater : ESP_055384_2310 ESP_055252_2310 (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 | 50.74 | 29.1 | -11. | 11.37 | 66.1 | 62.2 |
| Well-Preserved 14-Km Crater with Central Peak : ESP_055514_1930 ESP_063822_1930 (Interval in Earth days: 647) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 12.64 | 83.7 | 6.70 | -10.5 | 53.1 | 55.3 |
| Landforms in Majuro Crater : ESP_055501_1465 ESP_055646_1465 (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 | -33.0 | 84.6 | 4.48 | 23.51 | 59.3 | 56.1 |
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