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 Small Rayed Crater: ESP_025174_1660 ESP_028207_1660 (Interval in Earth days: 236)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-14.0	34.6	-2.7	6.91	51.7	58.6
Floor of Toro Crater: ESP_025344_1970 ESP_025067_1970 (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
17.00	71.7	-24.	0.616	41.9	38.4
Dunes: ESP_025054_1370 ESP_024988_1370 (Interval in Earth days: 5)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-42.5	73.9	5.41	22.31	69.5	67.6
Western Hecates Tholus Valleys: ESP_025275_2125 ESP_024985_2125 (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
32.22	149.	20.2	-5.23	37.6	40.0
Changes in Intracrater Dunes: ESP_025144_1420 ESP_024854_1420 (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
-37.7	136.	0.92	-24.0	67.3	64.7
Varied Crater Morphologies: ESP_025391_2325 ESP_025470_2325 (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
52.17	220.	4.72	24.81	45.1	43.0
Small Fresh Impact Crater: ESP_025115_2220 ESP_025616_2220 (Interval in Earth days: 39)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
41.47	198.	-4.7	16.78	42.6	39.3
Small Mounds in Chryse Planitia: ESP_025071_1995 ESP_025137_1995 (Interval in Earth days: 5)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
19.39	322.	-4.0	-23.5	38.6	40.7
Tongue-Shaped Flow Feature in Protonilus Mensae: ESP_025305_2225 ESP_025582_2225 (Interval in Earth days: 21)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
41.90	49.8	7.65	-9.56	41.0	41.7
Light-Toned Layered Deposits along Melas Chasma Floor: ESP_025178_1705 ESP_025244_1705 (Interval in Earth days: 5)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-9.57	283.	12.5	-10.2	48.1	50.4
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