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.
| East Melas Chasma Landslide Scarp: ESP_035951_1665 ESP_036307_1665 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.1 | 290. | -1.9 | 19.72 | 62.8 | 61.0 |
| Crater with Channels and Fans and Sinuous Ridges Near Distal Marte Vallis: ESP_035968_2045 ESP_036535_2045 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.01 | 182. | -8.3 | 7.886 | 46.2 | 47.5 |
| Possible Terraced Crater in Arcadia Planitia: ESP_035664_2235 ESP_036363_2235 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 43.02 | 197. | 5.86 | -8.77 | 42.4 | 47.7 |
| Inverted Channel Deep within Crater in Aeolis Dorsa: ESP_035600_1765 ESP_061090_1765 (Interval in Earth days: 1986) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.38 | 151. | 2.24 | 22.85 | 56.3 | 49.3 |
| Terraced Bullseye-Like Crater in Arcadia Planitia: ESP_035862_2195 ESP_035928_2195 (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 | 39.09 | 192. | 4.56 | -10.5 | 43.1 | 44.8 |
| Possible Chlorite-Bearing Knob in Northwest Hellas Region: ESP_035656_1530 ESP_035801_1530 (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 | -26.8 | 66.3 | -7.3 | 10.43 | 72.3 | 71.2 |
| Echus Montes: ESP_035938_1900 ESP_036993_1900 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.935 | 281. | 9.98 | -19.3 | 49.4 | 54.5 |
| Well-Preserved Impact Crater: ESP_035681_1920 ESP_043158_1920 (Interval in Earth days: 583) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.75 | 98.0 | 2.69 | 16.07 | 48.6 | 41.0 |
| South Kasei Valles Flow Front: ESP_035647_2065 ESP_036913_2065 (Interval in Earth days: 98) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.27 | 304. | 6.69 | -18.1 | 43.4 | 52.3 |
| Eastern Side of Terraced Deltaic Fan in Coprates Catena Trough: ESP_035832_1650 ESP_052368_1650 (Interval in Earth days: 1289) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.0 | 299. | -6.3 | -22.2 | 64.3 | 59.4 |
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