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.
| Wall of a Caldera on Summit of Ascraeus Mons: ESP_035306_1915 ESP_080288_1920 (Interval in Earth days: 3505) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.59 | 255. | 7.67 | 17.48 | 47.3 | 51.0 |
| Outflow Deposit from Hrad Vallis: ESP_035376_2145 ESP_034031_2145 (Interval in Earth days: 105) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.04 | 141. | 1.79 | 14.40 | 41.9 | 39.4 |
| Xanthe Terra Region: ESP_035528_1920 ESP_036873_1920 (Interval in Earth days: 105) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.66 | 315. | 0.16 | 11.08 | 48.5 | 51.2 |
| Small Lobe on Crater Floor at Terminus of Valley: ESP_035369_1940 ESP_035870_1940 (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 | 14.04 | 335. | 1.87 | 28.76 | 46.9 | 45.9 |
| North Polar Layered Deposit Exposure: ESP_035572_2665 ESP_036008_2665 (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 | 86.54 | 138. | 0.38 | -10.4 | 61.4 | 63.3 |
| Double-Terraced Crater next to Single-Terraced Crater in Arcadia Planitia: ESP_035545_2290 ESP_036455_2290 (Interval in Earth days: 71) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 48.74 | 206. | -4.8 | -18.2 | 43.8 | 50.5 |
| Faulted Layered Deposits in West Candor Chasma: ESP_035582_1745 ESP_036070_1745 (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 | -5.66 | 283. | -3.0 | -27.7 | 58.0 | 60.2 |
| Intracrater Dune Changes: ESP_035592_1900 ESP_035948_1900 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.747 | 8.03 | 3.25 | 18.32 | 49.3 | 48.9 |
| Candidate Landing Site for 2020 Mission: ESP_035304_1950 ESP_036148_1950 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 14.70 | 309. | 8.61 | -3.59 | 45.9 | 49.1 |
| Possible Terraced Crater in Arcadia Planitia: ESP_035585_2275 ESP_036495_2275 (Interval in Earth days: 71) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 47.36 | 193. | 1.38 | -13.4 | 43.1 | 50.2 |
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