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

Chasma Boreale Scarp with Possible Gypsum: PSP_001374_2650 PSP_001518_2650 (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
85.02	338.	-7.1	13.56	67.9	68.9
Northern Lowlands: PSP_002396_2345 ESP_020197_2345 (Interval in Earth days: 1387)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
54.37	186.	-1.5	-14.8	67.1	70.9
Lineated Valley Fill in Coloe Fossae : PSP_002902_2205 PSP_003245_2205 (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
40.17	53.8	3.42	-28.6	68.0	74.6
Dark Materials on Block in Olympus Mons Aureole : PSP_002461_1975 ESP_011282_1975 (Interval in Earth days: 687)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
17.06	217.	-4.5	16.43	56.5	56.4
Boulder Tracks with Boulders at Ends: PSP_001730_1740 PSP_002086_1740 (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
-5.87	16.4	-2.4	21.5	57.0	54.7
Gullies Possibly Produced by Snow/Ice Melting : PSP_003096_1375 PSP_003940_1375 (Interval in Earth days: 66)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-42.2	169.	-6.1	-22.4	59.0	47.6
White Rock Deposits: PSP_002033_1720 PSP_002099_1720 (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
-8.01	25.0	5.96	-17.5	56.7	58.4
Dark-Toned Unit Exposed atop Crater Ejecta in Meridiani Planum : PSP_002680_1825 PSP_003392_1825 (Interval in Earth days: 55)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
2.240	-0.3	7.78	29.45	55.2	53.5
Rayed Crater: PSP_001660_1950 PSP_002570_1950 (Interval in Earth days: 71)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
14.87	123.	-1.8	-15.8	51.0	57.9
Gullies on Very High Dune Slip Face in Russell Crater: PSP_001440_1255 PSP_001981_1255 (Interval in Earth days: 42)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-54.2	12.9	8.51	-8.06	85.6	80.5
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