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.
| A Heart in Ascraeus Mons: ESP_035807_1885 ESP_036862_1885 (Interval in Earth days: 82) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.176 | 258. | 9.65 | -14.9 | 50.0 | 54.0 |
| Slumping Terraces on a Crater Wall : ESP_035702_2270 ESP_035768_2270 (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 | 46.54 | 238. | 8.98 | -4.85 | 42.7 | 44.2 |
| Mission 2020: A Candidate Landing Site in Gusev Crater: ESP_035164_1655 ESP_036087_1655 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.5 | 175. | 6.33 | 27.49 | 61.9 | 61.5 |
| Ring of Cratered Cones: ESP_035098_2065 ESP_034808_2065 (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 | 26.23 | 170. | 22.2 | 0 | 40.4 | 41.6 |
| Graben South of Melas Chasma: ESP_035595_1640 ESP_043982_1640 (Interval in Earth days: 653) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.8 | 289. | 0.75 | -24.2 | 64.2 | 62.7 |
| Cratered Cones in Western Elysium Planitia: ESP_035521_1825 ESP_043987_1825 (Interval in Earth days: 659) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.375 | 146. | 8.82 | 22.29 | 52.4 | 48.1 |
| Exposure of North Polar Layered Deposits: ESP_035530_2665 ESP_044841_2665 (Interval in Earth days: 725) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 86.61 | 200. | 0.27 | -9.62 | 61.5 | 63.4 |
| Light-Toned and Swirly Deposits along Floor of Coprates Catena Trough: ESP_035410_1655 ESP_034988_1655 (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 | -14.5 | 299. | 6.08 | 21.52 | 62.7 | 60.1 |
| Wall of Orson Welles Crater: ESP_035594_1790 ESP_071042_1790 (Interval in Earth days: 2761) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.76 | 314. | 0 | 19.68 | 54.9 | 57.3 |
| Sediment Routing System in Aeolis Dorsa: ESP_035455_1780 ESP_036800_1780 (Interval in Earth days: 104) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.78 | 149. | 4.58 | 17.96 | 54.9 | 54.7 |
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