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

Relatively Fresh 1-Kilometer Diameter Crater in South Polar Region : ESP_013699_1055 ESP_013923_1055 (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
-74.1	130.	-4.9	10.22	57.2	58.2
Diverse Layers and Morphologies in North Rim of Hellas Planitia: ESP_013490_1525 ESP_058166_1530 (Interval in Earth days: 3481)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-27.3	64.2	-5.3	5.215	37.6	30.5
5 Kilometer Diameter Impact Crater Northwest of Mojave Crater: ESP_013968_1890 ESP_014390_1890 (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
8.866	328.	6.90	-3.58	44.6	40.6
South Polar Layered Deposits Exposed in Ultimum Chasma: ESP_013619_0990 ESP_013672_0990 (Interval in Earth days: 4)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-80.8	151.	18.0	4.365	60.2	61.5
Gullies Previously Identified in MOC Image: ESP_013849_1080 ESP_013981_1080 (Interval in Earth days: 10)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-71.9	354.	-7.6	-22.1	56.8	59.0
Raga Crater: ESP_014011_1315 ESP_014288_1315 (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
-48.1	242.	1.60	-18.1	41.9	45.6
Interesting Contrasts in Gully Morphology: ESP_014104_1360 ESP_021686_1360 (Interval in Earth days: 591)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-43.8	222.	3.50	25.74	40.1	42.0
Gullies in Gorgonum Chaos Mesas: ESP_012747_1425 ESP_013024_1425 (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
-37.0	189.	2.86	-20.5	46.1	44.2
Alcove in East Candor Chasma Layered Deposits: ESP_012809_1725 ESP_013310_1725 (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
-7.44	293.	-2.1	22.37	50.2	42.7
Fluidized Ejecta in the Kasei Valles Region: ESP_013204_2060 ESP_083253_2060 (Interval in Earth days: 5458)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
25.76	305.	0	16.06	65.4	67.6
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