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.
| Northern Mid-Latitude Terrain: ESP_078308_2145 ESP_078453_2145 (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 | 34.02 | 308. | -4.9 | 5.003 | 43.1 | 42.3 |
| Large Linear Features in Nilosyrtis Region Highlands: ESP_078541_2125 ESP_089248_2125 (Interval in Earth days: 834) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.01 | 67.3 | -8.6 | -23.0 | 43.4 | 49.3 |
| Crater-Edge Mounds in Chryse Planitia: ESP_078584_2055 ESP_078729_2055 (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 | 25.36 | 333. | -5.1 | 7.302 | 43.7 | 43.0 |
| Terrain Sample: ESP_078320_1825 ESP_078531_1825 (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 | 2.630 | 343. | 5.58 | -5.63 | 48.1 | 50.5 |
| Light Toned Outcrop in Arsinoes Chaos: ESP_078426_1715 ESP_086720_1715 (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 | -8.17 | 331. | -1.3 | -15.6 | 55.0 | 50.1 |
| Scarp with Yardangs: ESP_078326_1735 ESP_078260_1735 (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 | -6.21 | 181. | 4.36 | 27.22 | 52.6 | 50.2 |
| Northern Mid-Latitude Terrain: ESP_078339_2115 ESP_087200_2115 (Interval in Earth days: 690) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 31.13 | 181. | 3.47 | -7.62 | 42.2 | 42.6 |
| Jezero Crater Outcrop: ESP_078567_1985 ESP_080545_1985 (Interval in Earth days: 154) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.50 | 78.0 | 4.62 | 25.67 | 44.1 | 48.7 |
| Exposed Stratigraphy in Peraea Cavus Southern Wall: ESP_077960_1500 ESP_078171_1500 (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 | -29.7 | 95.5 | 24.1 | 12.30 | 61.6 | 65.1 |
| Well-Preserved 6-Kilometer Impact Crater South of Eos Chasma: ESP_078163_1610 ESP_081420_1610 (Interval in Earth days: 254) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.6 | 313. | 2.38 | 26.26 | 58.3 | 61.3 |
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