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.
| Southern Extension of Claritas Fossae: ESP_016647_1360 ESP_016792_1360 (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 | -43.7 | 277. | 2.88 | 16.79 | 76.6 | 77.4 |
| Gale Crater Layers in Northeast Section of Mound with Possible Sulfates: ESP_016586_1755 ESP_016731_1755 (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 | -4.64 | 138. | 0.77 | 18.24 | 49.8 | 49.8 |
| Possible Phyllosilicates in Her Desher Vallis: ESP_016527_1550 ESP_025032_1550 (Interval in Earth days: 663) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.8 | 311. | -6.8 | 7.004 | 62.1 | 56.3 |
| Layered Deposits along Floor of Melas Chasma: ESP_016673_1700 ESP_017952_1700 (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 | -9.67 | 284. | -5.2 | 5.092 | 53.8 | 59.7 |
| Cone Field in Phlegra Dorsa: ESP_016334_2090 ESP_016479_2090 (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 | 28.57 | 174. | -6.3 | 7.838 | 40.7 | 39.6 |
| Contact Between Different Lava Types on Olympus Mons: ESP_016820_1950 ESP_017888_1950 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 14.85 | 227. | -1.4 | 13.61 | 43.2 | 45.7 |
| Collapse Features on Hrad Vallis Mudflow: ESP_016467_2155 ESP_016533_2155 (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 | 35.13 | 141. | 0.42 | -15.9 | 41.1 | 42.4 |
| Upstream End of Eberswalde Crater Fan: ESP_016777_1560 ESP_018412_1560 (Interval in Earth days: 128) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -23.8 | 326. | -1.4 | 14.33 | 63.8 | 68.2 |
| Source Region for Branch of Auqakuh Vallis: ESP_016826_2080 ESP_016971_2080 (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 | 27.47 | 62.7 | -7.7 | 5.246 | 41.4 | 40.6 |
| Small Volcano in Northern Syria Planum: ESP_016318_1710 ESP_016951_1710 (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 | -8.76 | 254. | 6.70 | -9.92 | 48.9 | 55.9 |
Page 694 of 885 (8,850 images) | |||||