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 Dipping Layers in Ice-Affected Crater: ESP_080515_2115 ESP_080805_2115 (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 | 31.38 | 178. | -3.2 | 15.42 | 49.2 | 49.7 |
| Curvilinear Ridges on Floor of Shalbatana Vallis: ESP_080589_1885 ESP_080233_1885 (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 | 8.367 | 318. | 19.4 | -1.16 | 52.6 | 53.6 |
| High-Latitude Exposure of North Polar Layered Deposits: ESP_080218_2680 ESP_079956_2680 (Interval in Earth days: 20) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.72 | 307. | -7.8 | -23.6 | 65.0 | 64.2 |
| Dunes near Syrtis Major Planum Crater Ejecta: ESP_080242_1970 ESP_080308_1970 (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 | 16.58 | 72.6 | -8.3 | -24.6 | 51.1 | 52.7 |
| Ice-Rich Deposits in Arabia Terra: ESP_080204_2145 ESP_080138_2145 (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 | 34.14 | 27.7 | -8.5 | 6.219 | 47.6 | 46.0 |
| Grooves and Cataracts in Eos Chasma: ESP_080576_1665 ESP_080431_1665 (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 | -13.3 | 318. | -0.6 | -16.6 | 64.1 | 65.6 |
| Light-Toned Exposures in Margaritifer Terra: ESP_080417_1750 ESP_079296_1750 (Interval in Earth days: 87) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.13 | 339. | -20. | -8.88 | 61.4 | 59.2 |
| Baldet Crater Dune Changes: ESP_080229_2030 ESP_080295_2030 (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 | 22.68 | 65.8 | 1.70 | -15.0 | 48.5 | 50.2 |
| Juventae Chasma Interior Deposit Layers: ESP_080458_1755 ESP_080669_1755 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.62 | 297. | 11.5 | -0.14 | 58.9 | 59.5 |
| Possible Gully-Glacial Interaction in Utopia Planitia: ESP_080293_2195 ESP_080425_2195 (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 | 39.10 | 116. | 5.5 | -20.1 | 46.9 | 50.1 |
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