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

Debris Flow in Deuteronilus Mensae: ESP_016194_2260 ESP_016471_2260 (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
45.69	33.4	-1.8	-18.8	45.7	45.7
Well-Preserved 5-Kilometer Diameter Impact Crater in Amazonis Planitia: ESP_015924_2110 ESP_016768_2110 (Interval in Earth days: 66)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
30.90	207.	-2.0	-19.4	41.3	42.4
Light-Toned Material on Plateau North of Aurorae Chaos: ESP_016157_1745 ESP_016790_1745 (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
-5.39	330.	-6.7	-21.1	46.4	53.5
Recent Impact Crater with Dry Gullies: ESP_016056_1935 ESP_016478_1935 (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
13.20	204.	4.62	-6.65	39.1	42.3
Separated Distal Rampart from Tooting Crater: ESP_016280_2045 ESP_016425_2045 (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
24.24	208.	4.11	18.28	39.5	38.5
Light-Toned Outcrops and Unusual Ridges in Eastern Noctis Labyrinthus: ESP_015922_1720 ESP_016634_1720 (Interval in Earth days: 55)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-8.04	266.	-0.8	20.76	44.6	50.8
Ridge Near Olympus Mons: ESP_015976_1945 ESP_016899_1945 (Interval in Earth days: 72)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
14.11	229.	-5.1	12.21	39.4	42.7
Layered Rocks in Ius Chasma: ESP_016225_1730 ESP_018348_1730 (Interval in Earth days: 166)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-6.94	273.	0	-15.1	47.4	59.4
Marte Vallis Streamlined Landforms: ESP_016202_1895 ESP_016835_1895 (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
9.254	179.	5.93	-8.19	40.6	45.8
Well-Preserved Impact Crater: ESP_015905_2235 ESP_016182_2235 (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
42.91	3.36	3.72	-15.9	45.9	45.8
	Page 707 of 885 (8,850 images)