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

Ganges Mensa Layered Deposits: ESP_012993_1725 ESP_013059_1725 (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
-7.39	310.	-5.5	-26.0	48.5	49.3
Layered Bedrock on the Floor of an Impact Crater: ESP_012881_1880 ESP_013158_1880 (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
8.116	125.	0.85	-24.8	56.6	55.9
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
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
Olympus Mons Aureole: ESP_013273_2015 ESP_014262_2015 (Interval in Earth days: 77)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
21.19	220.	12.1	-1.21	60.9	49.4
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
Pit with Layered Walls in Mid-Latitude Mantling Unit: ESP_013951_1225 ESP_021731_1225 (Interval in Earth days: 606)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-57.3	82.3	2.27	-20.0	47.0	49.7
Terraced Double Crater in Margaritifer Sinus: ESP_014152_1505 ESP_014429_1505 (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
-29.3	350.	-5.5	-28.3	35.3	38.5
Circular Features: ESP_013460_1095 ESP_013302_1095 (Interval in Earth days: 13)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-70.4	165.	26.6	0.477	51.6	53.3
Exposure of South Polar Layered Deposits with Minor Faulting: ESP_012855_1065 ESP_012723_1065 (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
-73.2	132.	-7.1	7.21	58.4	58.8
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