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.
| Impact Crater Teetering on the Edge of a Canyon: ESP_017740_1680 ESP_025810_1680 (Interval in Earth days: 629) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.7 | 312. | 5.84 | -8.97 | 60.6 | 56.8 |
| Northern Hemisphere Gullies on a West-Facing Crater Slope: ESP_017405_2270 ESP_017827_2270 (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 | 46.67 | 90.1 | 7.09 | -4.59 | 41.7 | 43.0 |
| Polar Crater with Summer Ice: ESP_017510_2465 ESP_017945_2465 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 66.39 | 99.7 | -0.4 | 14.50 | 49.4 | 48.4 |
| Small Crater in Amazonis Planitia: ESP_017361_1830 ESP_018073_1830 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.024 | 219. | -6.7 | 4.499 | 51.3 | 52.3 |
| Slope Streaks in Lycus Sulci: ESP_017585_2080 ESP_025734_2080 (Interval in Earth days: 635) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 27.95 | 220. | -8.6 | 8.376 | 42.9 | 38.9 |
| Mini-Chaos in Crater Floor: ESP_017459_1990 ESP_053827_1990 (Interval in Earth days: 2834) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.80 | 61.3 | -4.8 | -27.4 | 44.6 | 46.9 |
| Possible Kieserite Deposit on Flanks of Hebes Mensa: ESP_017319_1785 ESP_017385_1785 (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 | -1.24 | 284. | 10.7 | -13.0 | 52.2 | 54.2 |
| Central Peak of an Impact Crater: ESP_017430_1910 ESP_018709_1910 (Interval in Earth days: 100) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.63 | 134. | -8.9 | 4.868 | 48.0 | 49.4 |
| Thermally-Anomalous Crater on Hrad Vallis Flow: ESP_017601_2145 ESP_018023_2145 (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 | 34.20 | 141. | 6.74 | -6.84 | 40.9 | 43.0 |
| Very Fresh Double Crater: ESP_017613_2195 ESP_017903_2195 (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 | 39.31 | 174. | -11. | 8.67 | 42.6 | 41.3 |
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