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.
| 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 |
| Mesa in Utopia Planitia: ESP_072817_2105 ESP_073107_2105 (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 | 30.31 | 89.3 | -8.4 | 14.89 | 59.1 | 60.6 |
| Hills in Phlegra Montes: ESP_073091_2170 ESP_081478_2170 (Interval in Earth days: 654) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.82 | 163. | 27.7 | 15.69 | 61.3 | 57.4 |
| Crater in Arabia Terra: ESP_072899_2205 ESP_072820_2205 (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 | 40.26 | 6.18 | 17.6 | -8.12 | 60.8 | 61.8 |
| 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 |
| Channel West of Idaeus Fossae: ESP_072809_2145 ESP_072954_2145 (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 | 34.10 | 305. | 5.91 | 16.08 | 58.8 | 59.8 |
| Candidate Recent Impact Site: ESP_073077_2155 ESP_073578_2155 (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 | 35.08 | 189. | -4.3 | 18.95 | 63.4 | 67.7 |
| 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 |
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