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.
| Landforms in Utopia Planitia : ESP_046521_2125 ESP_046666_2125 (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 | 32.43 | 87.2 | 5.50 | 18.37 | 55.5 | 56.4 |
| Eastern Rim and Ejecta of Resen Crater : ESP_046415_1520 ESP_046837_1520 (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 | -27.9 | 108. | 6.36 | -3.11 | 58.8 | 55.6 |
| Channels in a Crater Northeast of Hellas Planitia: ESP_046205_1515 ESP_046350_1515 (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 | -28.4 | 83.5 | -7.4 | 7.089 | 61.7 | 59.5 |
| Lobate Debris Apron in Northwest Argyre Region : ESP_046566_1335 ESP_046711_1335 (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 | -45.8 | 309. | -1.9 | 10.95 | 66.3 | 63.4 |
| 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 |
| Small Ridges in Rabe Crater : ESP_046576_1365 ESP_046998_1365 (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 | -42.9 | 35.4 | 8.28 | -2.65 | 64.0 | 58.9 |
| 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 |
| Light-Toned Material in Fresh Shallow Valleys : ESP_046458_2160 ESP_050928_2160 (Interval in Earth days: 348) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.49 | 8.31 | -8.2 | -25.0 | 56.9 | 44.0 |
| Well-Preserved 7-Kilometer Impact Crater : ESP_046334_2075 ESP_050883_2075 (Interval in Earth days: 355) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 27.00 | 154. | -7.3 | 5.524 | 52.7 | 37.9 |
| 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 |
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