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.
| Possible Mafic-Rich Armored Ejecta Deposits: ESP_074190_1195 ESP_074058_1195 (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 | -59.9 | 61.9 | -20. | 6.187 | 58.5 | 58.6 |
| Light-Toned Deposits in Iani Chaos: ESP_074087_1780 ESP_074021_1780 (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 | -2.04 | 342. | -6.0 | 19.68 | 56.1 | 54.4 |
| Tilted Layers in Electris Region: ESP_073948_1435 ESP_073882_1435 (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 | -36.2 | 181. | -8.9 | 7.304 | 54.7 | 54.4 |
| Channel along Edge of Crater: ESP_074028_1445 ESP_066233_1445 (Interval in Earth days: 607) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.1 | 156. | 7.22 | -5.51 | 52.2 | 41.6 |
| Phaethontis Region Slope Monitoring: ESP_074145_1390 ESP_073868_1390 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -40.7 | 204. | -14. | 6.12 | 53.0 | 55.6 |
| Small Delta or Fan: ESP_073983_1385 ESP_074260_1385 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -41.3 | 306. | 0.43 | -26.6 | 54.4 | 52.4 |
| Resistant Material in Olympus Mons Aureole Ridges: ESP_073920_1990 ESP_074065_1990 (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 | 18.79 | 218. | 1.52 | 19.57 | 64.0 | 63.0 |
| Lava-Crater Interaction in Elysium Planitia: ESP_073949_1860 ESP_074239_1860 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.812 | 148. | -1.0 | 25.38 | 58.9 | 56.1 |
| Well-Preserved 3-Km Impact Crater in Nereidum Montes: ESP_074035_1360 ESP_073890_1360 (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 | -43.6 | 326. | 11.5 | -7.18 | 53.3 | 56.9 |
| Channel Crossing Heavily Eroded Wrinkle Ridge: ESP_074146_1485 ESP_073790_1485 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -31.4 | 175. | -4.9 | -20.8 | 51.1 | 57.1 |
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