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.
| Banding at Margin of Circular Feature in CTX Image: ESP_017534_1690 ESP_087596_1685 (Interval in Earth days: 5459) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.1 | 177. | -8.5 | -24.7 | 60.5 | 60.6 |
| Small Crater in Amazonis Planitia: ESP_017361_1830 ESP_018073_1830 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.024 | 219. | -6.7 | 4.499 | 51.3 | 52.3 |
| Polar Crater with Summer Ice: ESP_017510_2465 ESP_017945_2465 (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 | 66.39 | 99.7 | -0.4 | 14.50 | 49.4 | 48.4 |
| Central Peak of an Impact Crater: ESP_017430_1910 ESP_018709_1910 (Interval in Earth days: 100) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.63 | 134. | -8.9 | 4.868 | 48.0 | 49.4 |
| Very Fresh Double Crater: ESP_017613_2195 ESP_017903_2195 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.31 | 174. | -11. | 8.67 | 42.6 | 41.3 |
| Crater Cut by Horst and Graben: ESP_017399_2185 ESP_017900_2185 (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 | 38.10 | 256. | -4.2 | 10.29 | 41.5 | 41.1 |
| Enigmatic Uplift on the Floor of Echus Chasma: ESP_017306_1815 ESP_018084_1815 (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 | 1.718 | 279. | 5.93 | -6.88 | 50.8 | 53.8 |
| Circular Features in Far Northern Reaches of Arcadia Planitia: ESP_017632_2475 ESP_018634_2475 (Interval in Earth days: 78) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 67.05 | 9.22 | -2.5 | 13.14 | 49.8 | 52.6 |
| Streamlined Landform with Benches in Kasei Valles System: ESP_017398_1970 ESP_017820_1970 (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 | 16.92 | 285. | 9.39 | -8.3 | 43.9 | 46.4 |
| Light-Toned Layered Deposits on Northern Edge of Hellas Planitia: ESP_017459_1500 ESP_018870_1500 (Interval in Earth days: 110) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -29.5 | 66.7 | 3.18 | -25.8 | 72.3 | 72.8 |
Page 694 of 900 (8,995 images) | |||||