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

Layer Exposure in Crater North of Meridiani Planum: ESP_015958_1835 ESP_016235_1835 (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
3.571	1.15	11.6	-17.7	39.8	44.4
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
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
Lineated Valley Floor Material in Terrain North of Arabia Region: ESP_016287_2205 ESP_077488_2205 (Interval in Earth days: 4769)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
40.04	15.5	-2.8	7.652	43.1	46.5
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
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
Exposure of Mid-Latitude Apron Interior by Younger Gully: ESP_015947_1370 ESP_051036_1370 (Interval in Earth days: 2734)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-42.5	308.	-3.0	-16.8	66.5	62.9
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
Syrtis Region: ESP_016048_2005 ESP_023907_2005 (Interval in Earth days: 613)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
20.48	62.8	0	-23.0	39.2	40.8
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