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.
| Rampart of Flow Ejecta: ESP_025260_1475 ESP_028293_1475 (Interval in Earth days: 237) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -32.3 | 209. | -5.1 | 5.684 | 65.2 | 67.7 |
| Fan Below Alcove Cut in Lower Southwest Gale Mound: ESP_025012_1745 ESP_033082_1745 (Interval in Earth days: 629) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.47 | 137. | -15. | 4.534 | 46.0 | 37.1 |
| Crater Flooded by Young Lava: ESP_025100_2040 ESP_025377_2040 (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 | 23.76 | 249. | 3.03 | -20.8 | 38.1 | 40.8 |
| Dunes: ESP_025054_1370 ESP_024988_1370 (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 | -42.5 | 73.9 | 5.41 | 22.31 | 69.5 | 67.6 |
| Fresh Gullies: ESP_025322_2400 ESP_026021_2400 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 59.45 | 302. | 5.47 | -8.94 | 49.3 | 46.8 |
| Proposed Future Landing Site in Ladon Valles: ESP_025295_1595 ESP_025783_1595 (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 | -20.4 | 329. | 22.4 | -2.40 | 55.6 | 62.0 |
| Small Fresh Impact Crater: ESP_025115_2220 ESP_025616_2220 (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 | 41.47 | 198. | -4.7 | 16.78 | 42.6 | 39.3 |
| Fluvial Fan on Crater Floor as Seen in THEMIS Image I03235002: ESP_025309_2155 ESP_024887_2155 (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 | 35.15 | 304. | -17. | -8.15 | 41.4 | 41.4 |
| Exposed Bedrock on Western Side of 42-Kilometer Crater Central Uplift: ESP_025304_1560 ESP_025027_1560 (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 | -23.5 | 88.5 | -22. | 4.349 | 60.6 | 55.5 |
| Erosional Features Near Head of Grjota Valles: ESP_025156_1965 ESP_025011_1965 (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 | 16.14 | 161. | 12.4 | -2.60 | 37.9 | 38.5 |
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