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

Light-Toned Layered Deposits Along Plains South of Ius Chasma: PSP_007786_1710 PSP_009935_1710 (Interval in Earth days: 167)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-8.74	276.	-4.8	20.55	52.9	58.8
Thinly-Banded Light-Toned Rock in Unnamed North Sinus Meridiani Crater: PSP_007084_1845 PSP_007440_1845 (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
4.433	2.80	3.48	-6.89	39.8	43.7
Terraced Fan Deposit in Tyras Vallis: PSP_008167_1885 PSP_008602_1885 (Interval in Earth days: 34)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
8.358	310.	-1.6	10.76	47.1	48.3
Fan in Aeolis Region: PSP_007975_1755 PSP_009623_1755 (Interval in Earth days: 129)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-4.65	154.	-4.9	5.617	52.4	57.8
Wall Layers of Tooting Crater: PSP_007907_2035 ESP_019115_2035 (Interval in Earth days: 873)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
23.18	208.	-2.3	5.434	41.6	48.0
Craters and Mounds in Utopia Planitia: PSP_007081_2190 PSP_009876_2190 (Interval in Earth days: 218)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
38.57	80.3	0.48	17.95	44.1	45.1
Middle Section of Northern Olympus Mons Basal Scarp: PSP_007089_2035 PSP_007946_2035 (Interval in Earth days: 67)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
23.25	223.	7.43	-6.64	38.8	42.1
Fine Layered Deposits in Capri Mensa: PSP_008088_1670 PSP_008378_1670 (Interval in Earth days: 23)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-12.8	310.	-6.2	5.9	58.3	59.7
Large Dunes Possibly of Aqueous Origin in Gale Crater: PSP_007356_1750 PSP_008147_1750 (Interval in Earth days: 62)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-5.19	137.	-4.1	6.367	46.5	53.3
Blocky Deposit and Valley Networks Along Melas Chasma Wallrock: PSP_007443_1705 PSP_007733_1705 (Interval in Earth days: 23)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-9.17	282.	-9.1	5.346	49.8	52.0
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