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

Layered Flow Ejecta in Terra Cimmeria: ESP_018379_1695 ESP_018880_1695 (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
-10.4	146.	6.62	27.95	60.0	57.5
North Polar Residual Cap: ESP_018289_2655 ESP_018593_2655 (Interval in Earth days: 24)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
85.19	34.7	5.01	-9.35	61.3	63.9
Two Distinct Surfaces along Mesa Wall in Deuteronilus Mensae: ESP_018225_2275 ESP_018146_2275 (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
47.18	22.7	5.82	-17.3	43.5	45.3
Lava Channel and Cataract in South-Central Elysium Planitia: ESP_018339_1820 ESP_018194_1820 (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
2.117	157.	-0.8	-16.4	53.3	54.4
Relatively Young Crater Ejecta and Apron in Deuteronilus Mensae: ESP_018423_2230 ESP_019056_2230 (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
42.74	18.1	3.74	-12.5	44.0	50.4
Fresh 3-Kilometer Diameter Crater near Margaritifer Region: ESP_018398_1715 ESP_025690_1715 (Interval in Earth days: 568)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-8.64	347.	5.56	-4.83	59.0	53.7
Fresh 2-Kilometer Diameter Impact Crater: ESP_018219_2155 ESP_078576_2155 (Interval in Earth days: 4702)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
35.25	189.	-0.7	11.46	43.1	41.8
Exposure of North Polar Layered Deposits in Area Not Well Observed: ESP_018376_2685 ESP_019113_2685 (Interval in Earth days: 57)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
88.32	200.	-20.	-13.4	65.1	71.7
Cracks and Fans on Dunes: ESP_018404_2610 ESP_018865_2610 (Interval in Earth days: 36)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
80.96	156.	6.25	24.73	59.0	62.0
Kasei Valles North Wall Terraces: ESP_018149_2060 ESP_018439_2060 (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
25.94	302.	-8.0	18.69	44.6	43.2
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