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.
| Mound with Linear Depression at Summit in Center of Crater: ESP_026042_2020 ESP_028574_2020 (Interval in Earth days: 198) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.91 | 93.1 | 2.80 | -9.54 | 41.2 | 53.6 |
| Small Fresh Crater on Northern Plains: ESP_026076_2320 ESP_026419_2320 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 51.66 | 236. | 24.6 | -3.11 | 40.7 | 42.9 |
| Newton Crater Valleys and Alluvial Fans: ESP_026012_1410 ESP_026078_1410 (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 | -38.7 | 199. | 4.09 | -15.0 | 76.7 | 78.1 |
| Layered Light-Toned Rounded Blocks in Melas Chasma: ESP_025811_1700 ESP_026312_1700 (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 | -10.2 | 284. | -7.9 | 16.99 | 55.8 | 57.1 |
| Valleys on Northern Flank of Hecates Tholus: ESP_026119_2135 ESP_026185_2135 (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 | 32.93 | 150. | -2.5 | -20.0 | 40.2 | 41.9 |
| Well-Preserved Impact Crater on Floor of Coprates Chasma: ESP_025982_1675 ESP_025626_1675 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.3 | 294. | 14.8 | 0 | 56.9 | 55.1 |
| Streamlined Forms in Elysium Planitia: ESP_025802_1960 ESP_026435_1960 (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 | 15.72 | 165. | 7.87 | -11.1 | 41.7 | 45.6 |
| Flow Margin Visible in Viking Image 731A38: ESP_026077_1770 ESP_027554_1770 (Interval in Earth days: 115) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.80 | 221. | -3.8 | -24.4 | 52.7 | 56.8 |
| Fresh Crater: ESP_025888_2365 ESP_025664_2365 (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 | 56.40 | 327. | 28.0 | 1.477 | 42.8 | 46.0 |
| Streamlined Layered Forms in Athabasca Valles: ESP_026198_1895 ESP_027042_1895 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.217 | 156. | -0.7 | -17.9 | 46.7 | 50.2 |
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