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

Lineated Valley Floor Material in Terrain North of Arabia Region: ESP_062519_2210 ESP_062730_2210 (Interval in Earth days: 17)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
40.42	15.4	4.31	-6.93	43.4	45.9
Polar Barchan Dunes: ESP_062237_2635 ESP_062198_2635 (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
83.64	121.	8.2	-7.26	59.3	59.9
High-Relief Cap Outlier Olympia Mensae: ESP_062542_2545 ESP_061988_2545 (Interval in Earth days: 43)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
74.36	97.4	0.78	18.48	55.6	51.9
Smooth Apron in Phlegra Montes: ESP_062540_2165 ESP_062751_2165 (Interval in Earth days: 17)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
36.4	162.	8.32	-3.60	43.0	45.5
Candidate Landing Site for 2020 Mission in Jezero Crater: ESP_062385_1990 ESP_062451_1990 (Interval in Earth days: 5)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
18.66	77.4	4.16	-19.3	45.3	47.5
Depressions near Mariner 9 Image DAS 6751223: ESP_062275_1810 ESP_062987_1810 (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
1.416	202.	9.46	-3.12	52.3	54.2
Ophir Chasma: ESP_062417_1755 ESP_062483_1755 (Interval in Earth days: 5)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-4.29	286.	0.50	-24.7	56.3	58.1
Sibiti Crater: ESP_062364_1675 ESP_062575_1675 (Interval in Earth days: 17)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-12.3	294.	5.62	-11.1	60.8	61.9
Fan Material in Crater within Southern Gale Crater: ESP_062317_1740 ESP_069651_1740 (Interval in Earth days: 571)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-5.81	137.	2.74	-7.32	56.9	60.1
Candidate Landing Site for 2020 and Sample Return Missions at Jezero Crater: ESP_062240_1985 ESP_062174_1985 (Interval in Earth days: 5)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
18.37	76.9	2.90	25.46	45.0	42.8
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