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

Gasa Crater Gully Monitoring: ESP_021584_1440 ESP_022217_1440 (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
-35.7	129.	-4.2	-23.6	44.3	38.4
Uplifted Bedrock in the Central Peak of an Impact Crater: ESP_020929_1360 ESP_021707_1360 (Interval in Earth days: 60)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-43.4	12.6	3.88	-7.43	55.0	44.1
Terrain between Aureum and Hydaspis Chaos: ESP_020416_1805 ESP_073151_1805 (Interval in Earth days: 4109)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
0.240	333.	-6.3	3.415	55.6	57.2
Layering in Yorktown Crater: ESP_020865_2030 ESP_065330_2030 (Interval in Earth days: 3465)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
22.90	311.	2.61	22.55	62.8	65.6
Wrinkle Ridges in Eastern Meridiani Planum: ESP_020705_1845 ESP_020850_1845 (Interval in Earth days: 12)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
4.228	2.86	-8.8	8.224	56.6	55.3
Mesa in Acidalia Planitia: ESP_020587_2250 ESP_047105_2250 (Interval in Earth days: 2066)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
44.76	338.	0.81	27.13	71.0	67.9
Ejecta of Very Well-Preserved Crater: ESP_020723_2235 ESP_064845_2235 (Interval in Earth days: 3438)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
43.26	225.	-4.6	28.28	72.1	71.8
Outcrop of Rhythmic Stratigraphy Southeast of Crommelin Crater: ESP_020534_1825 ESP_021523_1825 (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
2.225	350.	5.74	-9.90	54.9	53.6
Fresh 2-Kilometer Diameter Impact Crater Northwest of Hellas Planitia: ESP_020598_1490 ESP_020875_1490 (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
-30.8	47.1	7.13	-18.7	56.2	54.7
Aeolian Change Detection in Trouvelot Crater: ESP_020956_1955 ESP_020811_1955 (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
15.33	346.	16.4	0.7	58.8	59.5
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