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.
Possible Region of Past Ponded Water: ESP_014407_2045 ESP_020288_2045 (Interval in Earth days: 458) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.15 | 221. | 5.35 | 29.18 | 49.2 | 56.3 |
Trough Near Protonilus Mensae: ESP_014400_2200 ESP_022892_2200 (Interval in Earth days: 662) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.86 | 50.4 | 3.28 | -15.1 | 61.1 | 65.7 |
Stratigraphy of Crater Pedestal: ESP_014308_1135 ESP_020690_1135 (Interval in Earth days: 497) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -66.5 | 60.3 | -7.4 | 16.19 | 58.0 | 67.9 |
6-Kilometer Diameter Rayed Crater in Terra Sabaea: ESP_014400_1525 ESP_020703_1525 (Interval in Earth days: 491) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.3 | 59.1 | 4.96 | 17.81 | 35.1 | 53.4 |
Fresh 5-Kilometer Diameter Rayed Crater: ESP_014265_1570 ESP_020845_1570 (Interval in Earth days: 512) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -22.6 | 144. | 4.66 | -8.29 | 33.4 | 53.3 |
Layered Terrain between Aeolis and Zephyria Plana: ESP_014291_1770 ESP_020515_1775 (Interval in Earth days: 485) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.69 | 149. | 25.6 | 3.798 | 34.0 | 54.5 |
Exposures of Layered Rocks in Argyre Region: ESP_014167_1300 ESP_021947_1300 (Interval in Earth days: 606) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -49.7 | 302. | 8.10 | -18.2 | 43.7 | 44.1 |
Ferric Oxide-Rich Deposit in East Candor Chasma: ESP_014154_1730 ESP_014431_1730 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.75 | 292. | 5.69 | -21.1 | 35.2 | 35.9 |
Light-Toned Material in a Crater in Iani Chaos: ESP_013572_1795 ESP_022710_1795 (Interval in Earth days: 712) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.54 | 341. | -3.2 | 13.82 | 44.7 | 37.9 |
Exposure of Polar Layered Deposits Not Well Observed: ESP_013886_0875 ESP_022748_0875 (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 | -87.4 | 165. | 4.63 | 10.95 | 71.0 | 71.9 |
Page 683 of 851 (8,502 images) |