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

Ulysses Fossae Region Grabens: ESP_020314_1935 ESP_020815_1935 (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
13.21	236.	-1.2	20.75	56.5	57.1
Well-Preserved 11-Kilometer Diameter Crater in Tyrrhena Terra: ESP_020333_1710 ESP_028179_1710 (Interval in Earth days: 612)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-9.10	79.3	8.44	-4.88	54.6	57.4
Very Well-Preserved 15-Kilometer Diameter Crater in Thaumasia Planum: ESP_020167_1640 ESP_020312_1640 (Interval in Earth days: 12)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-15.6	292.	6.96	20.13	56.4	54.5
Light-Toned Rock: ESP_020234_1450 ESP_020946_1450 (Interval in Earth days: 55)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-34.6	266.	2.56	17.00	62.0	51.7
Potential Future Mars Landing Site in Noctis Labyrinthus: ESP_020089_1730 ESP_020511_1730 (Interval in Earth days: 33)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-6.93	261.	4.03	-15.6	55.3	55.8
Flow Structures in Noctis Region Trough: ESP_020313_1720 ESP_020735_1720 (Interval in Earth days: 33)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-8.08	265.	4.07	-12.9	54.9	54.8
Central Structure of Unnamed Crater near Thasis Region: ESP_020155_2130 ESP_020577_2130 (Interval in Earth days: 33)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
32.62	254.	4.51	-10.6	59.6	65.8
Ridges in Schiaparelli Crater: ESP_020322_1785 ESP_020955_1785 (Interval in Earth days: 49)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-1.36	18.1	15.4	-6.19	53.7	54.7
Bedrock Layers Exposed in West Proctor Crater: ESP_020256_1320 ESP_020889_1320 (Interval in Earth days: 50)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-47.6	28.2	-5.3	-20.9	67.7	58.9
Central Uplift of Crater within Larger Crater: ESP_020244_1805 ESP_029936_1805 (Interval in Earth days: 756)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
0.575	348.	0	15.21	55.0	52.9
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