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.
| South Polar Layered Deposits : ESP_057389_0925 ESP_057401_0925 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.5 | 93.6 | 7.25 | 21.26 | 65.2 | 63.8 |
| Channel within Larger Channel in Terra Cimmeria: ESP_057410_1445 ESP_065256_1445 (Interval in Earth days: 612) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.2 | 179. | 0.54 | 10.29 | 35.4 | 52.0 |
| Central Pit of 21-Kilometer Diameter Crater in Terra Sabaea : ESP_057151_1580 ESP_066514_1580 (Interval in Earth days: 730) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.9 | 47.2 | -0.3 | -20.4 | 38.8 | 41.1 |
| Candidate Landing Site for 2020 Mission in Gusev Crater : ESP_057265_1645 ESP_058386_1645 (Interval in Earth days: 87) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.3 | 175. | -5.9 | 5.6 | 39.4 | 29.3 |
| Valleys in a Crater in Terra Cimmeria: ESP_057490_1520 ESP_049169_1520 (Interval in Earth days: 649) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.7 | 155. | -2.2 | 7.232 | 34.3 | 30.5 |
| Layers in Arabia Terra : ESP_057231_1945 ESP_057719_1945 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 14.56 | 19.6 | -5.4 | 10.23 | 55.6 | 49.6 |
| Possible Wind Streaks and Multiple Flow Textures in Daedalia Planum : ESP_057131_1635 ESP_075014_1635 (Interval in Earth days: 1393) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -16.0 | 232. | -4.0 | 6.837 | 40.6 | 41.3 |
| Wall of 19-Kilometer Diameter Crater in Noachis Terra : ESP_057115_1590 ESP_058447_1590 (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 | -20.6 | 309. | 1.76 | 17.31 | 39.3 | 28.9 |
| Neighboring Gullies with Superposition Relationships : ESP_057100_2180 ESP_066199_2180 (Interval in Earth days: 709) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.85 | 354. | -22. | 3.404 | 74.3 | 74.6 |
| Candidate Paleobedforms South of Coprates Chasma : ESP_057445_1645 ESP_057511_1645 (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 | -15.3 | 301. | 5.93 | -10.6 | 36.4 | 36.8 |
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