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.
| Layering in Hellas Planitia: ESP_016299_1420 ESP_019978_1420 (Interval in Earth days: 287) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.4 | 57.0 | 7.21 | -12.1 | 67.3 | 67.2 |
| New Impact Site Formed Between January 2007 and May 2009: ESP_015949_1795 ESP_069449_1795 (Interval in Earth days: 4168) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.64 | 248. | -7.7 | 1.95 | 42.4 | 55.1 |
| Layered Bedrock in Central Uplift of a Large Crater: ESP_016132_1595 ESP_016765_1595 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -20.3 | 293. | 8.27 | -7.22 | 53.3 | 61.6 |
| Landslide Lobe in Eastern Ius Chasma: ESP_016172_1720 ESP_042334_1720 (Interval in Earth days: 2039) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.78 | 280. | 0 | -22.0 | 47.3 | 45.4 |
| Deep Bedrock Exposure in Melas Chasma: ESP_016264_1705 ESP_016897_1705 (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 | -9.22 | 288. | 7.41 | -7.19 | 48.5 | 55.6 |
| Triple Ricochet Crater in Ascuris Planum: ESP_016185_2215 ESP_016462_2215 (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 | 41.30 | 279. | -0.0 | -19.0 | 43.7 | 44.2 |
| Sinuous Ridge at Contact Between Lineated Valley Fill and Plains Material: ESP_016142_2240 ESP_080745_2240 (Interval in Earth days: 5033) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 43.67 | 13.6 | -3.2 | 20.12 | 45.2 | 49.8 |
| Unusual Flow-Ejecta Morphology: ESP_016226_1480 ESP_016371_1480 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -31.7 | 249. | 5.73 | 20.76 | 62.3 | 63.3 |
| Potential MSL Landing Site in Eberswalde Crater: ESP_016065_1560 ESP_016210_1560 (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 | -23.9 | 326. | -28. | -15.6 | 57.2 | 58.1 |
| Kunowsky Crater Central Peak with Strong Olivine Signature: ESP_016235_2370 ESP_016314_2370 (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 | 56.79 | 350. | 8.37 | 25.32 | 50.4 | 48.5 |
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