HiRISE | Stereo Pairs

Stereo Pairs

An explanation of stereo pairs and their use (PDF)

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.

Stereo Pair List (csv) Pairendipity Stereo Pairendipity CTX Stereo SPORCs

Possible Oudemans Crater-Related Deposits Emplaced into Valles Marineris: ESP_020880_1705 ESP_020814_1705 (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
-9.19	267.	-19.	3.696	54.4	53.0
Wrinkle Ridges in Eastern Meridiani Planum: ESP_020705_1845 ESP_020850_1845 (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
4.228	2.86	-8.8	8.224	56.6	55.3
Fresh and Well-Preserved Los Crater: ESP_020774_1445 ESP_024321_1445 (Interval in Earth days: 276)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-35.0	283.	-4.5	21.5	55.7	51.7
Fresh 2-Kilometer Diameter Impact Crater Northwest of Hellas Planitia: ESP_020598_1490 ESP_020875_1490 (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
-30.8	47.1	7.13	-18.7	56.2	54.7
Ejecta of Very Well-Preserved Crater: ESP_020512_2235 ESP_029571_2235 (Interval in Earth days: 706)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
43.22	225.	2.33	25.47	69.0	70.0
Crater Floor with Depressions Containing Circular Mesas: ESP_020535_1510 ESP_038020_1510 (Interval in Earth days: 1363)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-28.5	328.	-15.	-3.02	58.0	60.2
Outcrop of Rhythmic Stratigraphy Southeast of Crommelin Crater: ESP_020534_1825 ESP_021523_1825 (Interval in Earth days: 77)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
2.225	350.	5.74	-9.90	54.9	53.6
Bedding Features on Mound in Crater in Southern Arabia Terra: ESP_020836_1815 ESP_039495_1815 (Interval in Earth days: 1453)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
1.519	26.6	-7.6	7.514	55.8	51.2
Bedrock Exposure in Landslide Scarp: ESP_020879_1670 ESP_021657_1670 (Interval in Earth days: 61)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-12.9	293.	5.19	-7.68	52.2	46.1
Well-Preserved Large Impact Crater in Terra Sirenum: ESP_020777_1590 ESP_020843_1590 (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
-20.9	199.	5.03	-16.6	52.9	53.9
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