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.
| Mass Movement Feature as Seen in Image CTX Image: ESP_024669_1680 ESP_025170_1680 (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 | -11.8 | 141. | -3.1 | 17.74 | 44.2 | 49.0 |
| Boulder Slopes in Cerberus Fossae: ESP_024998_1900 ESP_024932_1900 (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 | 9.866 | 158. | -20. | 1.458 | 40.9 | 38.6 |
| Light-Toned Material along Coprates Chasma Ridge: ESP_024993_1670 ESP_025349_1670 (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 | -12.8 | 295. | 3.48 | 14.4 | 48.4 | 51.8 |
| Dunes and Ripples in Valles Marineris: ESP_025297_1730 ESP_025653_1730 (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 | -7.02 | 275. | 0 | 15.92 | 48.8 | 51.0 |
| Uplifted Jumble of Ancient Bedrock: ESP_025296_1535 ESP_025784_1535 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.3 | 305. | 1.24 | -22.8 | 61.0 | 67.4 |
| What is This Stuff?: ESP_024886_1765 ESP_025308_1765 (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 | -3.48 | 335. | 4.98 | -8.48 | 42.3 | 47.6 |
| Apollinaris Sulci Indurated Dunes: ESP_024483_1675 ESP_024127_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 | -12.6 | 178. | 23.0 | 6.505 | 40.2 | 37.0 |
| Material on Crater Floor West of Flammarion Crater: ESP_024435_2045 ESP_028391_2045 (Interval in Earth days: 308) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.44 | 46.5 | -3.9 | 10.17 | 38.7 | 50.5 |
| Faulted Layers in Becquerel Crater: ESP_024582_2015 ESP_024503_2015 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.36 | 352. | 10.4 | -21.2 | 36.6 | 39.3 |
| Channel in Lava Flow: ESP_024530_1570 ESP_042200_1570 (Interval in Earth days: 1377) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -22.6 | 338. | -5.9 | 11.68 | 48.5 | 49.2 |
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