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

Central Peak of Fesenkov Crater: PSP_007931_2020 ESP_024585_2020 (Interval in Earth days: 1298)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
21.68	273.	-8.3	-25.5	42.4	39.6
Eroded Craters on the Medusae Fossae Formation: PSP_008186_1840 PSP_009267_1840 (Interval in Earth days: 84)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
4.049	152.	-4.4	16.56	49.4	52.0
Layering in Eastern Central Peak of Oudemans Crater: PSP_007193_1700 PSP_008195_1700 (Interval in Earth days: 79)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-9.89	268.	4.49	-6.29	46.3	57.2
Gullies: PSP_007456_2140 ESP_016040_2140 (Interval in Earth days: 669)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
33.74	281.	-4.6	-22.7	41.7	43.6
Possible Sulfates in Ius Chasma: PSP_007509_1720 ESP_050839_1720 (Interval in Earth days: 3376)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-7.70	279.	-2.3	13.43	49.3	36.5
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
Fresh Double-Layered Ejecta Crater: PSP_007947_2350 PSP_009160_2350 (Interval in Earth days: 95)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
54.48	190.	0.23	-18.0	46.6	47.1
Dark Dunes Over Light-Toned Mega-Ripples Seen in MOC Image SP1-26004: PSP_007532_1905 PSP_008679_1905 (Interval in Earth days: 89)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
10.61	9.06	2.36	-9.87	41.8	49.2
Fresh 7-Kilometer Diameter Crater with Bright Rayed Ejecta: PSP_007731_2060 ESP_026310_2060 (Interval in Earth days: 1448)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
25.77	333.	1.95	28.52	40.6	38.7
Bacolor Crater Interior and Central Peak: PSP_007106_2135 PSP_009677_2135 (Interval in Earth days: 200)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
32.99	118.	0.49	-21.5	41.8	47.5
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