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.
A Fissure and Channel near Pavonis Mons: ESP_086934_1775 ESP_087435_1775 (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 |
-2.54 | 247. | -7.1 | 24.56 | 49.0 | 51.0 |
Ring-Shaped Mounds in Ceraunius : ESP_086815_2115 ESP_087092_2115 (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 |
31.79 | 249. | 16.7 | -7.37 | 40.6 | 42.5 |
Kasei Valles Scarps and Terraces: ESP_087921_2055 ESP_087855_2055 (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 |
25.07 | 301. | -29. | -8.33 | 46.5 | 44.4 |
USGS Dune Database Entry Number 1384-341: ESP_087637_1455 ESP_087703_1455 (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 |
-34.2 | 138. | 8.46 | -9.95 | 74.4 | 75.9 |
Light-Toned Fractured Material West of Nectaris Montes: ESP_087710_1655 ESP_087644_1655 (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 |
-14.4 | 303. | 1.75 | 21.48 | 61.6 | 59.9 |
Fan or Delta Deposits in Northeast Hargraves Crater: ESP_087916_2010 ESP_087072_2010 (Interval in Earth days: 65) | |||||
Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle |
20.98 | 75.9 | -5.5 | 6.04 | 45.3 | 41.6 |
Small Delta or Fan: ESP_087771_2065 ESP_087837_2065 (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 |
26.42 | 74.2 | -7.4 | -23.7 | 43.8 | 45.4 |
Crater in Arabia Terra: ESP_087747_2200 ESP_087681_2200 (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 |
39.57 | 7.75 | -7.8 | 6.691 | 43.3 | 42.0 |
Layers in Depression Walls Revealing Structure of Crater Ice Fill: ESP_087798_2270 ESP_087719_2270 (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 |
46.69 | 54.0 | -5.1 | -28.4 | 43.9 | 46.3 |
Layering in Western Lucus Planum: ESP_087912_1725 ESP_087978_1725 (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 |
-7.58 | 187. | 5.90 | -20.6 | 58.1 | 60.2 |
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