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.
| Arsia Mons Southern Caldera Wall Upper Flank and Caldera Floor : ESP_028872_1695 ESP_082280_1695 (Interval in Earth days: 4161) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -10.1 | 239. | 6.91 | -4.71 | 55.2 | 58.1 |
| Light-Toned Deposits in Ladon Valles Basin : ESP_028816_1605 ESP_029594_1605 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.2 | 329. | 6.81 | -3.96 | 57.8 | 53.2 |
| North-Central Endeavour Crater : ESP_028670_1780 ESP_028815_1780 (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 | -2.16 | 354. | -6.4 | 7.813 | 54.9 | 53.8 |
| Deformed Crater on Huygens Crater Floor : ESP_028826_1645 ESP_028760_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 | -15.4 | 56.3 | 5.64 | 27.53 | 56.7 | 55.2 |
| Crater Filled with Mantling Deposit in Far Eastern Acidalia Planitia : ESP_028628_2315 ESP_028694_2315 (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 | 51.20 | 54.1 | -4.9 | -17.8 | 61.8 | 64.0 |
| Exhumed Fan in Nilosyrtis Mensae : ESP_028680_2070 ESP_028825_2070 (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 | 26.90 | 76.8 | 7.55 | 18.85 | 53.9 | 54.5 |
| Rocky Massif : ESP_028737_1610 ESP_042807_1610 (Interval in Earth days: 1097) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.7 | 326. | 4.36 | -6.78 | 58.3 | 55.4 |
| Crater Ejecta Margin : ESP_028600_2255 ESP_046204_2255 (Interval in Earth days: 1371) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 45.03 | 99.4 | -3.0 | 7.704 | 58.8 | 55.5 |
| Olympus Mons Aureole Ripple Change Detection : ESP_028754_1975 ESP_028820_1975 (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 | 17.06 | 217. | 6.54 | -15.4 | 53.3 | 55.6 |
| Troughs and Mounds in Crater Near Reull Vallis : ESP_028640_1405 ESP_037224_1405 (Interval in Earth days: 669) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.3 | 98.8 | -6.1 | 8.772 | 68.8 | 71.7 |
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