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

Fresh Crater in Tyrrhena Terra: PSP_007172_1680 PSP_007462_1680 (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
-11.7	122.	-7.6	6.154	47.7	50.4
Light-Toned Rock in Central Peak of Alga Crater: PSP_007573_1555 PSP_007929_1555 (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
-24.3	333.	8.34	-3.28	59.4	64.1
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
Center of Mars: PSP_007361_1800 ESP_041909_1800 (Interval in Earth days: 2692)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-0.01	0.00	-0.1	20.55	44.1	35.7
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
Finely-Layered Fan Deposit of Possible Subaqueous Origin: PSP_007087_1700 PSP_007667_1700 (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
-9.81	283.	-7.7	22.30	45.8	50.5
Pits at the Head of the Hephaestus Fossae: PSP_007264_1975 PSP_007554_1975 (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
17.42	127.	-7.3	5.253	40.1	40.3
Geologic Contacts in Mangala Valles: PSP_007617_1750 PSP_007973_1750 (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
-4.85	209.	5.90	-6.28	48.4	52.6
8-Kilometer Diameter Rayed Crater: PSP_007757_1605 ESP_016196_1605 (Interval in Earth days: 658)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-19.2	348.	3.29	-18.5	58.6	55.2
Well-Preserved Crater Inside Williams Crater: PSP_007934_1610 PSP_007789_1610 (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
-18.9	195.	6.19	-1.34	60.0	58.9
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