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_073683_1645 ESP_073828_1645 (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 | -15.4 | 212. | -1.5 | 21.29 | 55.8 | 52.9 |
| Possible Clay-Rich Deposits in Crater Rims South of Her Desher Vallis: ESP_073864_1540 ESP_083253_1540 (Interval in Earth days: 732) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -25.8 | 312. | -2.6 | 6.656 | 54.3 | 46.9 |
| Barchanoid Dunes in Hellas Planitia: ESP_073543_1305 ESP_082075_1305 (Interval in Earth days: 665) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -49.0 | 79.2 | -4.1 | 7.99 | 64.0 | 68.0 |
| Cliffs of Crumbling, Layered Sediments: ESP_072533_1680 ESP_078309_1680 (Interval in Earth days: 450) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.9 | 288. | -0.4 | -20.4 | 60.3 | 57.4 |
| Small Crater Exposed via Erosion: ESP_073113_1735 ESP_073047_1735 (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 | -6.27 | 293. | -16. | 7.203 | 59.1 | 57.3 |
| Region Dubbed Troy: ESP_073472_0950 ESP_073471_0950 (Interval in Earth days: 0) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -85.0 | 259. | -8.9 | 18.63 | 82.6 | 80.4 |
| Branched Curved Ridge Feature in THEMIS Image I07922005: ESP_073448_1240 ESP_073593_1240 (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 | -55.4 | 153. | -4.4 | 7.946 | 67.9 | 64.6 |
| Serpentine-Bearing Mound in Ariadnes Colles: ESP_073157_1450 ESP_073513_1450 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -34.8 | 173. | 5.66 | 17.35 | 63.5 | 58.3 |
| Embayment Relations around Ridge: ESP_073179_2090 ESP_073469_2090 (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 | 28.65 | 285. | -3.0 | 25.24 | 62.4 | 63.2 |
| Small Delta or Fan: ESP_073462_1815 ESP_073739_1815 (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 | 1.685 | 122. | 6.30 | -14.2 | 57.4 | 58.9 |
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