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 Shield Volcano North of Noctis Labyrinthus: ESP_066572_1825 ESP_066783_1825 (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 | 2.527 | 259. | -1.9 | 21.85 | 47.7 | 43.9 |
| Elongating Linear Dunes in Argyre Planitia: ESP_066808_1330 ESP_066610_1330 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -46.8 | 305. | 2.41 | 28.89 | 43.0 | 40.3 |
| Enigmatic Channel in Syrtis Major: ESP_066803_1955 ESP_084000_1955 (Interval in Earth days: 1340) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 15.18 | 74.3 | -3.1 | -22.9 | 52.7 | 57.6 |
| Features in Iani Chaos: ESP_066503_1795 ESP_066569_1795 (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 | -0.27 | 342. | 7.35 | -6.95 | 46.4 | 46.7 |
| Features in Mamers Valles: ESP_066528_2215 ESP_075391_2215 (Interval in Earth days: 690) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 41.30 | 14.3 | 5.69 | -4.18 | 74.0 | 73.2 |
| Scarp Fronted Deposit in South Gunjur Crater: ESP_066774_1795 ESP_067526_1795 (Interval in Earth days: 59) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.32 | 146. | 8.48 | 17.64 | 43.5 | 38.5 |
| Lobate Features in Southeast Koval Sky Crater: ESP_066600_1485 ESP_066811_1485 (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 | -31.3 | 219. | 6.22 | 26.63 | 38.3 | 36.2 |
| Ridges West of Vernal Crater: ESP_066872_1860 ESP_057720_1860 (Interval in Earth days: 713) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.102 | 353. | -16. | 6.368 | 47.5 | 44.0 |
| Channel-Like Features in Cerberus Region: ESP_066589_1935 ESP_075175_1935 (Interval in Earth days: 668) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 13.50 | 153. | 9.00 | 7.223 | 53.3 | 54.5 |
| Relatively Pristine 7-Kilometer Crater with Gullies: ESP_066597_1435 ESP_066465_1435 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.3 | 302. | 1.02 | 24.41 | 39.4 | 37.9 |
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