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.
| Mesa near Mawrth Vallis: ESP_077450_2055 ESP_077951_2055 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.02 | 336. | -8.9 | 3 | 42.3 | 41.5 |
| Crater with Gullies: ESP_077101_1375 ESP_077312_1375 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -41.9 | 147. | -1.0 | 17.92 | 58.0 | 60.4 |
| Pasted-on Material on Crater Ejecta: ESP_077346_1845 ESP_077135_1845 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.419 | 294. | 18.5 | -6.08 | 38.2 | 38.9 |
| Central Peak Pit of 38-Kilometer Diameter Crater in Noachis Terra: ESP_077160_1450 ESP_085454_1450 (Interval in Earth days: 646) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -34.8 | 336. | -0.9 | 12.53 | 54.3 | 44.9 |
| Mesa in Southern Utopia Planitia: ESP_077300_2050 ESP_076258_2050 (Interval in Earth days: 81) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.51 | 108. | 7.3 | -8.80 | 41.1 | 49.6 |
| Flow Margin in Elysium Planitia: ESP_077364_1855 ESP_078076_1855 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.628 | 164. | 0 | 15.68 | 39.7 | 44.1 |
| Layers along Graben Wall of Arsia Mons Flank: ESP_077124_1725 ESP_077058_1725 (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 | -7.48 | 236. | -8.9 | 5.849 | 40.9 | 39.1 |
| Channels in Rahway Valles: ESP_076981_1890 ESP_076770_1890 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.810 | 175. | 11.0 | -7.15 | 37.2 | 38.5 |
| Gully Monitoring and Topography: ESP_076936_1360 ESP_085019_1360 (Interval in Earth days: 630) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -43.8 | 330. | 4.64 | 28.22 | 56.2 | 43.1 |
| Interaction Between Cone and Ejecta : ESP_076922_2250 ESP_077832_2250 (Interval in Earth days: 71) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.42 | 341. | -3.8 | 8.962 | 55.0 | 46.2 |
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