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.
| Dune Interaction with Residual Polar Ice: ESP_080689_2600 ESP_080781_2600 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.05 | 94.1 | -8.1 | 6.268 | 64.9 | 65.0 |
| Dune Interaction with Residual Polar Ice: ESP_080662_2620 ESP_080688_2620 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 81.96 | 107. | -6.9 | 7.38 | 65.5 | 64.9 |
| Southern Dunes: ESP_080784_2550 ESP_080626_2550 (Interval in Earth days: 13) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 74.86 | 18.4 | 8.83 | -7.19 | 62.2 | 61.5 |
| Acidalia Planitia Impact Crater Exposing Layered Materials: ESP_080681_2125 ESP_080826_2125 (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 | 32.22 | 326. | -7.1 | 2.814 | 50.7 | 51.0 |
| Inlet Valley: ESP_080967_1990 ESP_079912_1990 (Interval in Earth days: 82) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.71 | 78.2 | 3.35 | 15.98 | 52.7 | 47.5 |
| Paleolake Crosscut by Shalbatana Vallis: ESP_080945_1900 ESP_081433_1900 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.748 | 319. | 6.16 | -27.4 | 54.1 | 58.8 |
| Trough Cutting across Wrinkle Ridge in Labeatis Fossae: ESP_080788_2095 ESP_086260_2095 (Interval in Earth days: 426) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 29.03 | 284. | -5.6 | 4.56 | 51.4 | 42.0 |
| 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 |
| 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 |
| 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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