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.
| North-Pole-Facing Deposit in Crater: ESP_087303_2255 ESP_087448_2255 (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 | 45.12 | 247. | -5.0 | 7.456 | 44.4 | 43.0 |
| Overlapping Debris Aprons on Floor of Ganges Chasma: ESP_087538_1720 ESP_087683_1720 (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 | -8.01 | 318. | -4.5 | 16.00 | 56.9 | 56.4 |
| Crater near Cerberus Fossae: ESP_087280_1890 ESP_087636_1890 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.029 | 158. | 7.69 | 23.79 | 45.6 | 46.3 |
| Alluvial Fan in Eos Chasma: ESP_087037_1660 ESP_088105_1660 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.7 | 316. | -5.3 | 25.28 | 55.9 | 61.5 |
| Crater Wall with Potential Chloride Deposit Outcrop: ESP_086817_1465 ESP_090153_1465 (Interval in Earth days: 260) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -33.3 | 205. | -2.0 | 16.07 | 65.8 | 68.4 |
| Exposed Ancient Crust in Coprates Chasma: ESP_086866_1650 ESP_080550_1650 (Interval in Earth days: 492) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.9 | 305. | -10. | 25.78 | 55.0 | 63.2 |
| High-Latitude Crater: ESP_086952_2425 ESP_088099_2425 (Interval in Earth days: 90) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 62.05 | 104. | 3.58 | 29.37 | 52.9 | 45.4 |
| Crater Wall with Potential Chloride Deposit Outcrop: ESP_086962_1470 ESP_090087_1470 (Interval in Earth days: 243) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -32.9 | 205. | 9.32 | 29.33 | 66.7 | 67.8 |
| Jarosite-Bearing Terrain in Northern Nili Fossae: ESP_086927_2070 ESP_088483_2070 (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 | 26.80 | 74.9 | -6.0 | -23.3 | 42.0 | 46.9 |
| Volcanic Vent Southeast of Pavonis Mons: ESP_086802_1790 ESP_087079_1790 (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 | -1.03 | 249. | 8.99 | -22.0 | 45.9 | 50.7 |
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