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

Flow Features on Ice-Rich Plateau on Malea Patera: ESP_083276_1165 ESP_083144_1165 (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
-63.1	53.5	-7.0	15.29	55.0	55.2
Eroded Landform in Chryse Planitia: ESP_083121_1940 ESP_083767_1940 (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
13.87	312.	-4.9	22.98	62.5	56.4
Scour Pit Island in Southeastern Part of Medusae Fossae Formation: ESP_083046_1795 ESP_083191_1795 (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
-0.69	201.	-0.6	13.40	55.9	53.9
Channel Entering Crater: ESP_082956_1395 ESP_083378_1395 (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
-40.3	143.	4.73	-7.28	51.9	46.6
Hillslope Morphologies in Crater: ESP_082945_1510 ESP_083011_1510 (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
-28.8	83.4	-4.8	-26.4	51.8	52.7
Ariadnes Colles: ESP_083100_1450 ESP_083588_1450 (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
-34.6	171.	3.68	-22.4	49.2	44.5
Crater with Steep Slopes: ESP_083268_1375 ESP_083624_1375 (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
-42.0	266.	-6.4	2.905	48.4	43.1
Channel in Valley near Tyrrhena Patera: ESP_083076_1590 ESP_083142_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
-20.6	104.	3.93	-19.6	50.0	51.0
Juventae Chasma Interior Deposit Layers: ESP_082937_1760 ESP_082357_1760 (Interval in Earth days: 45)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-4.16	297.	8.05	-7.44	54.7	58.4
Small Delta or Fan: ESP_083042_1885 ESP_083675_1885 (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
8.626	309.	6.05	-18.1	59.4	56.7
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