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 Geyser Locale : ESP_049370_0945 ESP_040615_0945 (Interval in Earth days: 682) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -85.4 | 103. | 4.68 | -8.56 | 69.6 | 71.9 |
| Fan Deposit with Incised Channels : ESP_049616_1735 ESP_049682_1735 (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 | -6.29 | 190. | 4.80 | -15.2 | 30.9 | 32.2 |
| Exposure of South Polar Layered Deposits : ESP_049408_0920 ESP_049222_0920 (Interval in Earth days: 15) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.0 | 178. | 13.3 | 23.03 | 72.4 | 68.7 |
| Exit Breach in Well-Preserved Crater : ESP_049306_2160 ESP_049860_2160 (Interval in Earth days: 43) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.79 | 7.54 | 6.11 | -20.4 | 61.2 | 54.9 |
| Nilosyrtis Mensae : ESP_049686_2145 ESP_059497_2145 (Interval in Earth days: 764) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.25 | 74.3 | 6.05 | 16.85 | 54.6 | 42.1 |
| Multiple Curved Ridges at End of Valley in Protonilus Mensae : ESP_049621_2210 ESP_049766_2210 (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 | 40.50 | 47.8 | 4.69 | 20.26 | 60.7 | 57.8 |
| Mcmurdo Crater : ESP_049308_0955 ESP_049202_0955 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -84.4 | 0.90 | -8.0 | 7.236 | 68.8 | 66.4 |
| Western Rim and Ejecta of Resen Crater : ESP_049329_1520 ESP_049896_1520 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.9 | 108. | -3.1 | 22.04 | 31.4 | 33.4 |
| Small Crater on South Polar Layered Deposits : ESP_049637_0920 ESP_049860_0920 (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 | -87.9 | 40.6 | 11.9 | 23.22 | 75.5 | 78.0 |
| Faults in Zephyria Planum : ESP_049446_1800 ESP_057424_1800 (Interval in Earth days: 621) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.01 | 151. | -1.1 | 27.25 | 34.8 | 42.2 |
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