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 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
Impressive Central Peak: PSP_007555_1965 ESP_024354_1965 (Interval in Earth days: 1309)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
16.11	100.	-5.7	-26.8	41.4	38.6
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
Potential Fan Deposit in Ritchey Crater with Clays: PSP_007363_1510 PSP_008365_1510 (Interval in Earth days: 78)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-28.4	308.	3.89	-7.30	59.7	71.0
Hellas Planitia: PSP_007715_1420 ESP_016022_1420 (Interval in Earth days: 647)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-37.4	57.6	8.36	23.98	70.4	62.4
Crater in the Adamas Labyrinthus Region Seen in THEMIS Image V21701005: PSP_007713_2170 PSP_009862_2170 (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
36.45	103.	-4.4	10.64	41.9	45.6
Deposits in Kasei Valles: PSP_007970_2015 ESP_033551_2015 (Interval in Earth days: 1993)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
21.06	287.	-0.6	17.86	42.0	36.8
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
Fault Relays in the Cerberus Fossae: PSP_007645_1885 PSP_007856_1885 (Interval in Earth days: 16)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
8.465	164.	-5.5	-23.3	43.9	46.8
Cut Crater in Ganges Chasma: PSP_008101_1710 ESP_016263_1710 (Interval in Earth days: 636)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-8.91	314.	-5.3	21.95	55.9	47.3
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