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.
| Interesting Crater Ejecta in Columbus Crater: ESP_016861_1505 ESP_017639_1505 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -29.3 | 193. | 1.16 | -12.7 | 68.3 | 73.7 |
| Very Large Pit Crater in Daedalia Planum: ESP_016411_1605 ESP_024481_1605 (Interval in Earth days: 629) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.4 | 237. | 0 | -21.9 | 56.8 | 47.0 |
| Aureum Chaos: ESP_016803_1770 ESP_088144_1770 (Interval in Earth days: 5559) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.11 | 334. | -3.6 | -16.2 | 51.1 | 57.8 |
| Terrain South of Newcomb Crater: ESP_016736_1520 ESP_068970_1525 (Interval in Earth days: 4070) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.6 | 5.59 | 4.65 | -7.50 | 65.7 | 63.9 |
| Possible MSL Rover Landing Site in Northeast Syrtis Region: ESP_016575_1980 ESP_016509_1980 (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 | 17.81 | 77.2 | -17. | 2.958 | 42.7 | 40.7 |
| Eroded Material Adjacent to Cerberus Fossae: ESP_016506_1890 ESP_017495_1890 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.114 | 160. | 2.89 | -11.8 | 42.9 | 49.1 |
| Central Uplift and Olivine-Rich Ponded Material in Elorza Crater: ESP_016659_1710 ESP_017081_1710 (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 | -8.77 | 304. | 10.5 | -3.93 | 52.2 | 56.4 |
| Crater in Acidalia Planitia: ESP_016841_2340 ESP_017830_2340 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 53.72 | 7.48 | 5.69 | -6.67 | 45.4 | 44.9 |
| Cerberus Fossae: ESP_016822_1865 ESP_017600_1865 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.281 | 173. | 2.06 | -11.4 | 46.2 | 50.8 |
| Possible Landslide Triggered by Impact: ESP_016386_1475 ESP_016531_1475 (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 | -32.4 | 201. | 1.20 | 16.67 | 65.1 | 65.9 |
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