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.
| 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 |
| Lava Channels in Tartarus Montes: ESP_035586_2050 ESP_036364_2050 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.73 | 170. | -1.9 | 13.12 | 44.3 | 46.0 |
| Cratered Cones in Western Elysium Planitia: ESP_035521_1825 ESP_043987_1825 (Interval in Earth days: 659) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.375 | 146. | 8.82 | 22.29 | 52.4 | 48.1 |
| Characterize Distal Alluvial Fan Slopes: ESP_035468_1755 ESP_045398_1755 (Interval in Earth days: 773) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.70 | 154. | 6.76 | -20.1 | 56.5 | 54.1 |
| Exposure of North Polar Layered Deposits: ESP_035530_2665 ESP_044841_2665 (Interval in Earth days: 725) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 86.61 | 200. | 0.27 | -9.62 | 61.5 | 63.4 |
| Candidate Future Landing Site in Jezero Crater: ESP_035563_1990 ESP_035629_1990 (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 | 18.61 | 77.9 | 10.8 | -9.74 | 45.0 | 46.8 |
| 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 |
| 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 |
| Graben South of Melas Chasma: ESP_035595_1640 ESP_043982_1640 (Interval in Earth days: 653) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.8 | 289. | 0.75 | -24.2 | 64.2 | 62.7 |
| Exposure of North Polar Layered Deposits: ESP_035568_2655 ESP_036306_2655 (Interval in Earth days: 57) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 85.31 | 268. | -3.7 | 5.673 | 60.5 | 64.0 |
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