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.
| Alluvial Fans in Southwestern Mojave Crater: ESP_046275_1870 ESP_051958_1870 (Interval in Earth days: 443) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.160 | 326. | 5.60 | 25.31 | 49.5 | 40.4 |
| Fresh Shallow Valleys and Fans in North Arabia Terra: ESP_046247_2160 ESP_050361_2160 (Interval in Earth days: 320) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.83 | 8.50 | -4.9 | -20.4 | 53.8 | 48.7 |
| Transition from Inverted to Depressed Channel in Terra Sirenum : ESP_046346_1430 ESP_060126_1430 (Interval in Earth days: 1074) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.6 | 193. | 8.10 | -1.33 | 63.5 | 62.1 |
| Floor of Uzboi Vallis Near Nirgal Vallis: ESP_046249_1495 ESP_055255_1495 (Interval in Earth days: 701) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -30.0 | 322. | -8.1 | -27.3 | 62.2 | 63.0 |
| Streamlined Islands in Marte Vallis : ESP_046386_1885 ESP_046531_1885 (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 | 8.480 | 177. | -14. | 0.964 | 51.7 | 51.1 |
| Mesa Island in East Acidalia Planitia : ESP_046498_2250 ESP_046788_2250 (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 | 44.70 | 353. | 7.48 | 27.40 | 60.0 | 63.0 |
| Complex Ridge in Utopia Planitia : ESP_046323_2155 ESP_055197_2155 (Interval in Earth days: 692) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.32 | 93.8 | -8.0 | 8.45 | 54.9 | 55.3 |
| Ridge in Utopia Planitia : ESP_046349_2115 ESP_046415_2115 (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 | 31.34 | 103. | 5.70 | -12.7 | 52.9 | 55.2 |
| Eos Chasma: ESP_046302_1630 ESP_046658_1630 (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 | -16.9 | 313. | -3.8 | 6.507 | 55.8 | 53.2 |
| Lava Flow and Channels near Olympica Fossae: ESP_046555_2005 ESP_046700_2005 (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 | 20.43 | 241. | -8.0 | 8.018 | 53.6 | 53.7 |
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