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.
| Impacts from MSL Tungsten Blocks and Cruise Stage: ESP_029245_1755 ESP_031869_1755 (Interval in Earth days: 204) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.40 | 136. | 1.29 | -18.0 | 54.3 | 35.6 |
| Colorful Fractured Bedrock in Ritchey Crater: ESP_029542_1510 ESP_029964_1510 (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 | -28.5 | 308. | 14.3 | 3.043 | 53.3 | 49.1 |
| Cerberus Fossae : ESP_028954_1900 ESP_029376_1900 (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 | 9.810 | 158. | 6.13 | -8.14 | 54.0 | 57.1 |
| Graben with Gullied Walls : ESP_028953_1430 ESP_029019_1430 (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 | -36.7 | 192. | -7.3 | -25.4 | 64.1 | 64.8 |
| Layers in Lower Southwest Candor Chasma in MOC Image R08-02264 : ESP_028910_1740 ESP_029622_1740 (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 | -6.17 | 282. | -5.8 | 7.178 | 55.4 | 52.9 |
| Active Geyser Locale : ESP_028984_0945 ESP_028983_0945 (Interval in Earth days: 0) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -85.4 | 104. | -0.2 | 24.96 | 89.5 | 87.4 |
| 20-Kilometer Crater in Meridiani Planum Exposing Layers : ESP_029092_1770 ESP_029804_1770 (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 | -2.96 | 353. | -8.5 | 3.934 | 55.2 | 53.2 |
| Ridges and Valley and Flow Fronts in CTX Image D03_028235_1829_XN_02N011W: ESP_029013_1830 ESP_031215_1830 (Interval in Earth days: 171) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.723 | 348. | 3.34 | 11.42 | 54.2 | 43.8 |
| Possible Gullies in Graben : ESP_028913_1580 ESP_029335_1580 (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 | -21.7 | 201. | 4.96 | -8.40 | 58.1 | 55.9 |
| Multiple Geologic and Geomorphic Units in Contact : ESP_029151_1695 ESP_029296_1695 (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 | -10.4 | 182. | 4.21 | 20.99 | 54.6 | 52.7 |
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