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 |
| 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 |
| 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 |
| Ridged Flow-Like Features in Deuteronilus Mensae: ESP_080916_2230 ESP_080837_2230 (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 | 42.50 | 26.9 | 5.87 | -18.6 | 52.7 | 54.0 |
| Streamlined Landforms Adjacent to Shalbatana Vallis: ESP_080655_1890 ESP_080721_1890 (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 | 9.021 | 317. | 5.31 | -18.5 | 53.6 | 55.7 |
| Crater Ejecta Crosscut by Channels in Aeolis Dorsa: ESP_080727_1735 ESP_080437_1735 (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 | -6.32 | 152. | 19.9 | -7.28 | 58.7 | 61.1 |
| Crater in Arabia Terra: ESP_080864_2145 ESP_080363_2145 (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 | 34.04 | 7.53 | 10.5 | -7.04 | 50.7 | 48.5 |
| 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 |
| Traverse Ramp in Eastern Coprates Chasma: ESP_080761_1640 ESP_080339_1640 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.6 | 306. | 2.60 | 15.19 | 64.6 | 64.9 |
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