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.
| Channel Carved Into Scarp within Isidis Planitia: ESP_013186_1945 ESP_013252_1945 (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 | 14.55 | 78.4 | -2.7 | -24.1 | 58.1 | 58.9 |
| Relatively Fresh 1-Kilometer Diameter Crater in South Polar Region : ESP_013699_1055 ESP_013923_1055 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -74.1 | 130. | -4.9 | 10.22 | 57.2 | 58.2 |
| Saheki Crater Alluvial Fan Layering Exposed in Eastern Portion of Crater: ESP_012949_1580 ESP_013226_1580 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.7 | 73.0 | 0.82 | -26.3 | 44.2 | 42.9 |
| Layered Alunite-Kaolinite Deposit: ESP_013775_1490 ESP_021924_1490 (Interval in Earth days: 635) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -30.4 | 202. | 4.83 | 29.52 | 34.9 | 36.8 |
| 5 Kilometer Diameter Impact Crater Northwest of Mojave Crater: ESP_013968_1890 ESP_014390_1890 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.866 | 328. | 6.90 | -3.58 | 44.6 | 40.6 |
| Alcove in East Candor Chasma Layered Deposits: ESP_012809_1725 ESP_013310_1725 (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 | -7.44 | 293. | -2.1 | 22.37 | 50.2 | 42.7 |
| Possible Blocky Deposit in Melas Chasma: ESP_013508_1665 ESP_014141_1665 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.2 | 289. | 6.08 | -18.0 | 39.2 | 35.6 |
| Gullied Crater and Central Uplift: ESP_013799_1310 ESP_057842_1310 (Interval in Earth days: 3432) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -48.8 | 270. | 2.07 | 15.09 | 41.2 | 37.9 |
| Landslides at the Edge of the South Polar Layered Deposits: ESP_013026_1080 ESP_013224_1080 (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 | -71.9 | 143. | -8.2 | -28.8 | 56.2 | 56.7 |
| High-Latitude Gullies: ESP_012803_1185 ESP_012948_1185 (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 | -61.1 | 106. | -7.2 | 1.666 | 52.9 | 50.6 |
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