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.
| Ponded Ejecta Next to Flow Features in Bakhuysen Crater Ejecta : ESP_047236_1555 ESP_047526_1555 (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 | -24.0 | 14.6 | -5.0 | 21.39 | 51.0 | 46.0 |
| Crater in Noachis Terra : ESP_047249_1290 ESP_050084_1290 (Interval in Earth days: 221) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -50.5 | 22.8 | 4.07 | -13.9 | 57.7 | 52.8 |
| Colorful Layered Bedrock in Eroded Crater in Terra Sirenum : ESP_047150_1520 ESP_041282_1520 (Interval in Earth days: 457) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.8 | 203. | -5.4 | 15.87 | 52.5 | 38.6 |
| Mesa and Mounds in Utopia Planitia : ESP_047299_2155 ESP_047589_2155 (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 | 35.08 | 86.0 | 3.78 | 21.88 | 66.5 | 67.9 |
| Geryon Montes Wall Landforms : ESP_047279_1720 ESP_047345_1720 (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 | -7.74 | 278. | -1.4 | -24.6 | 50.6 | 52.2 |
| Landforms in Utopia Planitia : ESP_047048_2095 ESP_055276_2095 (Interval in Earth days: 641) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 29.24 | 99.8 | 5.69 | -7.83 | 60.7 | 55.8 |
| Lobes and Low-Lying Bakhuysen Crater Ejecta Deposits : ESP_047170_1580 ESP_047605_1580 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.5 | 16.4 | -7.3 | 27.91 | 51.5 | 44.5 |
| Intersecting Channels near Olympica Fossae: ESP_045091_2045 ESP_044326_2045 (Interval in Earth days: 59) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.30 | 249. | -4.6 | 20.49 | 42.8 | 39.4 |
| A Human Bird’s Eye View of Mars: PSP_006633_2010 PSP_007556_2010 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.99 | 74.4 | 4.70 | -20.5 | 38.8 | 42.1 |
| Possible Rhythmic Bedding in Medusae Fossae Formation : ESP_046742_1695 ESP_046887_1695 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -10.5 | 180. | -9.8 | 8.738 | 52.9 | 51.0 |
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