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.
| Stunning Outcrop in Nilosyrtis Mensae: ESP_088681_2160 ESP_088892_2160 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.47 | 65.6 | -5.2 | -14.7 | 44.7 | 46.4 |
| Fan in Crater North of Nepenthes Mensae: ESP_088705_1815 ESP_088916_1815 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 1.468 | 133. | 4.91 | -7.86 | 54.8 | 55.9 |
| Steep Sandy Slopes in Coprates Chasma: ESP_088554_1660 ESP_088620_1660 (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 | -13.7 | 298. | 11.2 | -14.2 | 63.4 | 65.0 |
| Kasei Valles Alluvial Fans: ESP_088633_2040 ESP_088778_2040 (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 | 23.55 | 298 | -6.4 | 3.817 | 46.5 | 46.1 |
| Ridged Flow-Like Features in Deuteronilus Mensae: ESP_088445_2225 ESP_088511_2225 (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 | 42.33 | 26.8 | 8.67 | -8.24 | 42.8 | 44.5 |
| Jezero Crater: ESP_088562_1985 ESP_089208_1985 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.47 | 77.4 | -8.9 | 15.11 | 48.1 | 47.9 |
| Fan-Shaped Feature in Ismenius Lacus: ESP_088485_2145 ESP_088696_2145 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.95 | 17.5 | -4.9 | -15.7 | 44.2 | 45.9 |
| Structure of Viscous Flow Feature Exposed by Ice Degradation: ESP_088510_2220 ESP_088431_2220 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 41.58 | 51.9 | 11.0 | -13.2 | 42.7 | 44.7 |
| Flow Entering Fretted Terrain Valley: ESP_088735_2170 ESP_088669_2170 (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 | 36.59 | 32.1 | -14. | 4.335 | 45.7 | 43.8 |
| North Polar Residual Cap Topography: ESP_088751_2685 ESP_089016_2685 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 88.39 | 276. | -17. | -26.2 | 64.2 | 66.2 |
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