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.
| Crater within Kasei Valles: ESP_034830_2025 ESP_036241_2025 (Interval in Earth days: 110) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.14 | 290. | 3.80 | -7.00 | 42.2 | 47.6 |
| Trough with Channels in Elysium Fossae: ESP_034519_2100 ESP_035020_2100 (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 | 29.50 | 140. | 4.29 | 15.4 | 40.2 | 40.3 |
| Fan and Channel Forms in Memnonia Sulci Region: ESP_034768_1695 ESP_035757_1695 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -10.5 | 186. | 6.76 | -7.65 | 57.1 | 61.5 |
| Candidate Future Landing Site: ESP_034808_1655 ESP_034874_1655 (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 | -14.3 | 175. | 1.98 | -21.3 | 60.1 | 62.0 |
| Gully Without Apron: ESP_034628_2340 ESP_035063_2340 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 53.73 | 41.1 | -2.0 | 18.22 | 45.1 | 42.5 |
| Possible Terraced Crater in Arcadia Planitia: ESP_034504_2305 ESP_034636_2305 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 50.19 | 186. | 5.28 | -22.2 | 43.6 | 45.6 |
| Contact of Medusae Fossae Formation with Flank of Apollinaris Mons: ESP_034597_1730 ESP_034663_1730 (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 | -6.92 | 174. | 12.3 | -12.5 | 53.2 | 55.4 |
| Light-Toned Stratified Materials in Eastern Candor Chasma: ESP_034896_1725 ESP_036452_1725 (Interval in Earth days: 121) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.55 | 292. | -3.8 | 11.60 | 56.7 | 58.2 |
| Lava Textures inside Kasei Valles: ESP_034724_2065 ESP_035568_2065 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.17 | 303. | 4.53 | -23.0 | 41.0 | 45.8 |
| Ejecta Flow over and around Pre-Existing Obstacles: ESP_034690_2175 ESP_035336_2175 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.19 | 150. | 7.52 | 28.85 | 40.3 | 39.0 |
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