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.
| Lava Filling Craters in Elysium Planitia: ESP_080529_1895 ESP_080674_1895 (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 | 9.230 | 159. | -7.8 | 3.279 | 54.3 | 53.7 |
| Dune Monitoring in Northern Mid-Latitude Crater: ESP_080539_2425 ESP_080618_2425 (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 | 62.07 | 238. | -7.6 | 7.316 | 55.0 | 54.6 |
| Landslide near Kasei Valles: ESP_080273_2085 ESP_079996_2085 (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 | 28.13 | 303. | 5.79 | 17.72 | 47.4 | 45.1 |
| Floor of East Coprates Chasma: ESP_080471_1650 ESP_080972_1650 (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 | -15.0 | 304. | 7.33 | 20.06 | 64.8 | 62.3 |
| Dune Monitoring in Northern Mid-Latitude Crater: ESP_080576_2395 ESP_080286_2395 (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 | 59.33 | 302. | 24.5 | 7.497 | 51.7 | 50.5 |
| Dune Interaction with Residual Polar Ice: ESP_080398_2605 ESP_079884_2605 (Interval in Earth days: 40) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.56 | 98.8 | 21.6 | 8.03 | 60.3 | 57.7 |
| 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 |
| Streamlined Landforms adjacent to Shalbatana Vallis: ESP_080299_1895 ESP_080444_1895 (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 | 9.172 | 318. | -13. | 12.02 | 54.3 | 52.6 |
| A Fissure Vent East of Olympus Mons: ESP_080579_1955 ESP_080790_1955 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 15.48 | 232. | 5.92 | -6.42 | 51.4 | 53.1 |
| Eroded Sedimentary Rock Layers: ESP_080568_1670 ESP_080779_1670 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.7 | 176. | -1.1 | -14.0 | 63.8 | 64.2 |
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