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.
| Possible Inverted Channels on Fan Feature: ESP_073059_1600 ESP_073204_1600 (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 | -20.0 | 327. | 7.39 | 22.17 | 59.8 | 57.6 |
| Strata in Butte in Chryse Planitia: ESP_072953_2060 ESP_073243_2060 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.76 | 336. | -0.2 | 24.76 | 59.1 | 59.9 |
| Small Delta or Fan: ESP_072815_1725 ESP_072960_1725 (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 | -7.62 | 148. | -1.0 | 12.96 | 58.5 | 57.1 |
| Possible Future Landing Site for Mars Sample Return: ESP_072567_1990 ESP_072857_1990 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.58 | 76.9 | -11. | 11.73 | 55.6 | 56.0 |
| A Large New Slump in Eos Chasma: ESP_071886_1640 ESP_069895_1640 (Interval in Earth days: 155) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.7 | 315. | -3.4 | 12.83 | 64.3 | 65.6 |
| Dark Patches Formed by Craters: ESP_071661_1570 ESP_071806_1570 (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 | -22.8 | 339. | -7.9 | 6.204 | 69.7 | 68.0 |
| Layered Sedimentary Rocks in Candor Chasma: ESP_072599_1735 ESP_073588_1735 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.33 | 284. | 7.09 | -6.72 | 57.9 | 57.2 |
| Deposits in Iani Chaos: ESP_072676_1775 ESP_073520_1775 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.24 | 342. | 0.62 | -26.6 | 57.3 | 59.6 |
| Chaos-Like Valley Southwest of Deuteronilus Mensae: ESP_072622_2160 ESP_072833_2160 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.47 | 11.6 | 2.93 | -6.19 | 57.0 | 60.5 |
| Monitor Vaduz Crater: ESP_072635_2185 ESP_072701_2185 (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 | 38.26 | 15.7 | 7.55 | -10.5 | 57.4 | 59.8 |
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