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.
| Channel in Maadim Vallis : ESP_045951_1560 ESP_046162_1560 (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 | -23.5 | 176. | 7.72 | -1.89 | 60.0 | 59.2 |
| Valley with Flows in Noachis Terra : ESP_045853_1525 ESP_046565_1525 (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 | -27.2 | 333. | -6.9 | 5.379 | 63.7 | 57.2 |
| Basin with Lava Fill in Southern Elysium Planitia : ESP_045938_1775 ESP_046149_1775 (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 | -2.57 | 167. | 18.6 | 9.184 | 49.8 | 50.6 |
| Crater with Blocky Interior in Marte Vallis : ESP_045977_1920 ESP_046267_1920 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.83 | 183. | -6.5 | 20.42 | 48.6 | 48.0 |
| Candidate Landing Site for 2020 Mission in Jezero Crater : ESP_045994_1985 ESP_046060_1985 (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 | 18.42 | 77.4 | 3.48 | -18.2 | 47.5 | 49.9 |
| Syria Planum Bedform and Albedo Changes : ESP_046080_1655 ESP_046502_1655 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.2 | 252. | 22.2 | 7.064 | 53.8 | 53.2 |
| 1-Kilometer Diameter Crater : ESP_046065_2260 ESP_046355_2260 (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 | 45.84 | 295. | -5.3 | 13.65 | 54.8 | 57.7 |
| East Coprates Montes Dark Fans : ESP_045907_1665 ESP_046619_1665 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.3 | 297. | -2.1 | 12.58 | 55.8 | 52.1 |
| Thin Layers in Eroded Crater Southwest of Bamberg Crater : ESP_046142_2165 ESP_046643_2165 (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 | 36.34 | 355. | -6.1 | 12.42 | 52.7 | 58.2 |
| Light-Toned Surface in Valley in CTX Image : ESP_046011_1620 ESP_046723_1620 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -17.8 | 338. | -6.0 | 11.19 | 57.7 | 52.7 |
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