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.
| Pitted Cones in Chryse Planitia : ESP_058723_2160 ESP_059000_2160 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.84 | 327. | 4.89 | -20.5 | 52.8 | 50.7 |
| Scamander Vallis : ESP_058800_1965 ESP_058589_1965 (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 | 16.03 | 28.4 | -4.5 | 7.472 | 38.7 | 40.1 |
| Smooth Region in Phlegra Montes : ESP_058729_2170 ESP_059006_2170 (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 | 36.54 | 162. | 7.97 | -17.3 | 53.1 | 50.9 |
| Hunt for Ancient Impact Craters Near Nili Fossae : ESP_058772_2025 ESP_058706_2025 (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 | 22.32 | 72.3 | -7.1 | 14.88 | 43.0 | 42.4 |
| Channels in Nilokeras Mensae : ESP_058816_2100 ESP_076765_2100 (Interval in Earth days: 1398) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 29.61 | 309. | 1.56 | -8.48 | 47.1 | 47.6 |
| Gullies in Crater in Terra Cimmeria : ESP_058901_1335 ESP_067341_1335 (Interval in Earth days: 657) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -45.9 | 158. | 1.39 | 29.38 | 48.4 | 45.6 |
| Troughs in Acidalia Planitia : ESP_058987_2245 ESP_058565_2245 (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 | 43.98 | 319. | -7.2 | 8.327 | 56.1 | 61.5 |
| Well-Exposed Ejecta Blanket at Kontum Crater : ESP_058896_1480 ESP_058962_1480 (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 | -31.7 | 292. | 3.30 | -18.2 | 38.8 | 41.1 |
| Valleys in Crater Northeast of Argyre Planitia : ESP_058934_1500 ESP_059356_1500 (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 | -29.6 | 335. | 2.03 | -13.0 | 38.2 | 45.5 |
| Gullies from Layers in Asimov Crater in MOC Image R1600339 : ESP_058788_1320 ESP_067703_1320 (Interval in Earth days: 694) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -47.5 | 4.65 | -4.2 | 8.752 | 48.1 | 53.5 |
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