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

Lava Flow Margin in Echus Chasma: ESP_013271_1810 ESP_013693_1810 (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
1.211	279.	2.08	-12.7	48.9	44.8
Mound on Nili Patera Floor: ESP_013582_1895 ESP_020940_1895 (Interval in Earth days: 574)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
9.139	67.3	1.63	-17.6	49.9	58.9
Differential Erosion of Light-Toned Stratigraphy in Melas Chasma: ESP_013640_1710 ESP_012928_1710 (Interval in Earth days: 56)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-8.93	285.	8.51	-10.3	39.1	48.9
Light-Toned Outcrop in Lower Coprates Chasma Wall: ESP_013231_1690 ESP_013732_1690 (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
-10.9	292.	1.57	23.81	43.7	36.2
Valleys and Layering along Melas Chasma: ESP_013561_1705 ESP_013983_1705 (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
-9.60	283.	-0.8	-18.8	40.4	37.5
East Slope of Asimov Crater Central Pit: ESP_013189_1330 ESP_013835_1330 (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
-46.8	5.12	-5.7	20.37	43.1	39.0
3 Kilometer Diameter Crater on Edge of South Polar Layered Deposits: ESP_013344_0990 ESP_013463_0990 (Interval in Earth days: 9)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-80.7	112.	-6.3	-22.2	60.8	62.4
Strike Slip Fault in Amazonis Planitia: ESP_012799_1990 ESP_013076_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
18.75	203.	1.92	-21.6	63.2	63.0
Light-Toned Material in a Crater in Terra Cimmeria: ESP_013750_1440 ESP_021543_1440 (Interval in Earth days: 608)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-35.8	166.	-2.2	19.05	36.5	43.0
Enigmatic Crater Fill: ESP_013055_1010 ESP_012818_1010 (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
-78.8	68.2	20.0	-4.42	58.4	61.9
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