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.
| Inverted Channel in Cusus Valles: ESP_067833_1960 ESP_067965_1960 (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 | 16.05 | 49.8 | 5.88 | -3.77 | 43.8 | 44.2 |
| Knob on Acidalia Mensa: ESP_067928_2275 ESP_068073_2275 (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 | 47.36 | 336. | -13. | 22.80 | 61.5 | 57.4 |
| Layered Deposits in West Candor Chasma: ESP_067785_1755 ESP_067983_1755 (Interval in Earth days: 15) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.63 | 283. | -10. | -25.6 | 40.8 | 43.3 |
| Cones in Chryse Planitia: ESP_068087_1990 ESP_067691_1990 (Interval in Earth days: 31) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.98 | 323. | -21. | 5.62 | 46.4 | 45.9 |
| Crater Floor Outcrop: ESP_067980_2160 ESP_063970_2160 (Interval in Earth days: 312) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.60 | 0.43 | -22. | -12.2 | 54.5 | 59.7 |
| Terrain in Cydonia Region: ESP_067848_2205 ESP_068970_2200 (Interval in Earth days: 87) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.15 | 358. | -1.9 | -16.2 | 57.0 | 50.7 |
| Gullies Eroding Thick Mantling Deposits: ESP_067903_1370 ESP_073574_1370 (Interval in Earth days: 442) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -42.6 | 308. | -5.4 | 22.27 | 54.7 | 59.3 |
| Hills in Phlegra Montes: ESP_067842_2165 ESP_072656_2165 (Interval in Earth days: 375) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.26 | 162. | 0.51 | 13.88 | 54.4 | 56.7 |
| Positive Relief Feature near South Pole: ESP_067842_0920 ESP_067803_0920 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.9 | 193. | 25.0 | 19.34 | 84.0 | 83.9 |
| Candidate Recent Impact Site: ESP_068033_1700 ESP_068561_1700 (Interval in Earth days: 41) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.76 | 357. | 5.83 | -4.07 | 41.9 | 48.9 |
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