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.
| From Ares 3 to Ares 4: ESP_042014_1760 ESP_042647_1760 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.96 | 15.1 | 3.24 | -28.0 | 38.9 | 47.4 |
| Western Medusa Fossae Formation: Dust and Dunes: ESP_041864_1745 ESP_050725_1745 (Interval in Earth days: 691) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.43 | 150. | 2.13 | 25.91 | 37.9 | 33.3 |
| Candidate ExoMars Landing Site in Hypanis Valles: ESP_041937_1920 ESP_042003_1920 (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 | 11.88 | 314. | 16.7 | -5.73 | 35.9 | 37.9 |
| Channel Containing Streamlined Forms Near Anseris Mons: ESP_041972_1490 ESP_042117_1490 (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 | -30.7 | 86.3 | -8.6 | 5.165 | 52.1 | 53.5 |
| Layered Materials on Floor of Ritchey Crater: ESP_041977_1515 ESP_042122_1515 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.2 | 308. | -2.2 | 11.68 | 50.1 | 51.5 |
| Geologic Contact between Fluvial Deposits in Aeolis Dorsa: ESP_041943_1745 ESP_050303_1745 (Interval in Earth days: 652) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.30 | 154. | -6.0 | 6.611 | 39.3 | 31.5 |
| Hydrated Materials within Orson Welles Crater: ESP_041924_1790 ESP_052130_1790 (Interval in Earth days: 795) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.97 | 313. | -19. | 7.429 | 39.3 | 47.1 |
| Daedalia Planum Lava Flows: ESP_041940_1570 ESP_042006_1570 (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 | -22.7 | 237. | 4.90 | -18.3 | 46.0 | 48.4 |
| Convoluted Folds in Light-Toned Deposits along Ius Chasma Floor: ESP_041899_1725 ESP_042321_1725 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.47 | 275. | -0.2 | -19.6 | 39.0 | 45.0 |
| Winding Valley in Sinus Sabaeus Region: ESP_041974_1740 ESP_042119_1740 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.17 | 27.5 | 3.38 | 18.36 | 39.2 | 39.5 |
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