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

Dunes Dubbed Redondo: ESP_063313_2545 ESP_071583_2545 (Interval in Earth days: 645)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
74.49	288.	-7.5	7.525	64.6	57.9
Possible Impact Melt Deposits in a Multiple Impact Structure: ESP_062296_1840 ESP_062586_1840 (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
4.036	349.	5.58	22.88	51.2	50.4
Dynamic Activity in a Crater North of Antoniadi Crater : ESP_023261_2065 ESP_023327_2065 (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
26.12	57.0	-1.8	-18.8	49.3	49.4
Pollywog Craters on Mars: ESP_061768_2200 ESP_062045_2200 (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
39.79	0.03	-0.9	-11.2	40.7	42.4
Layered Bedrock in the Central Uplift of Betio Crater: ESP_016805_1565 ESP_017583_1565 (Interval in Earth days: 61)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-23.1	281.	3.96	-9.12	63.3	68.9
Candidate Landing Site for 2020 and Sample Return Missions at Jezero Crater: ESP_062662_1990 ESP_062952_1990 (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
18.61	77.2	-29.	-12.5	49.4	49.2
High-Latitude Crater with Patterned Ground: ESP_062992_2475 ESP_063216_2475 (Interval in Earth days: 18)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
67.07	55.0	-2.5	13.10	56.3	57.9
High-Latitude Lobate Slope Features: ESP_062735_2495 ESP_062959_2495 (Interval in Earth days: 18)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
69.49	232.	-6.9	7.134	55.1	56.4
Layering in Medusae Fossae Formation: ESP_062632_1715 ESP_062843_1715 (Interval in Earth days: 17)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-8.41	177.	-7.3	-22.0	59.3	60.3
Dunes Dubbed Hazar South: ESP_062970_2550 ESP_062838_2550 (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
74.99	293.	-6.2	5.004	60.4	58.2
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