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

Gullies in Nereidum Montes: ESP_065515_1400 ESP_065937_1400 (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
-39.4	312.	-1.0	25.03	49.9	42.5
Layers in Crater: ESP_065354_1890 ESP_065974_1890 (Interval in Earth days: 49)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
8.820	20.8	-6.1	-22.4	60.8	58.8
Candidate Recent Impact Site: ESP_065360_1900 ESP_065703_1900 (Interval in Earth days: 27)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
10.06	217.	-7.7	-26.7	61.5	61.7
Gullied Slope: ESP_065466_1455 ESP_065809_1455 (Interval in Earth days: 27)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-34.1	209.	-3.7	-19.0	50.3	47.1
Flow-Like Feature in Chryse Planitia: ESP_065356_1995 ESP_065422_1995 (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
19.37	323.	5.19	-11.2	65.1	66.3
Gullies: ESP_065408_1420 ESP_073546_1420 (Interval in Earth days: 634)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-37.6	351.	6.35	29.29	50.5	57.6
USGS Dune Database Entry 2579-573: ESP_065438_1225 ESP_065517_1225 (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
-57.3	257.	-4.7	21.47	55.7	52.7
Layers in Valles Marineris Wall: ESP_065449_1675 ESP_066135_1675 (Interval in Earth days: 53)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-12.1	309.	-0.0	-25.1	52.4	47.6
Gullied Slope: ESP_065493_1415 ESP_065427_1415 (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
-38.3	193.	-8.5	6.271	50.6	50.4
Flat Layered Deposits and Candidate Exit Breach in Small Young Crater: ESP_065414_1495 ESP_065480_1495 (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
-30.3	186.	8.30	-7.95	49.9	50.3
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