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

Alluvial Fans in Crater: ESP_019489_1510 ESP_025291_1510 (Interval in Earth days: 452)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-28.5	84.0	4.07	-20.3	66.3	63.8
Claritas Fossae Region with Possible Serpentine: ESP_019509_1530 ESP_019654_1530 (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
-26.8	258.	-8.0	9.024	66.0	63.8
Small Fan in Amenthes Fossae Region: ESP_019264_1895 ESP_019897_1895 (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
9.201	101.	5.29	-10.3	51.1	54.7
Rim and Ejecta of Very Fresh 7-Kilometer Diameter Crater in Arcadia Region: ESP_019547_2335 ESP_024848_2335 (Interval in Earth days: 413)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
53.29	288.	5.88	-21.5	58.3	51.5
Well-Preserved 6-Kilometer Diameter Impact Crater: ESP_019371_1700 ESP_020571_1700 (Interval in Earth days: 94)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-9.81	63.1	4.37	-11.4	57.7	55.3
Lava Vent with Channels: ESP_019325_1960 ESP_019391_1960 (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
15.69	235.	7.19	-14.6	49.9	52.1
Diverse Lithologies in Central Uplift of Stokes Crater: ESP_019380_2360 ESP_019604_2360 (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
55.59	171.	-16.	10.82	58.7	59.7
Monitoring of Pits and Fractures in Deuteronilus Mensae: ESP_019504_2240 ESP_019570_2240 (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
43.81	25.2	1.42	-13.1	54.7	56.8
Crater in Sinus Sabaeus Region: ESP_019386_1700 ESP_020019_1700 (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
-10.0	13.6	3.93	-10.0	57.8	57.1
Exhumed Light-Toned Deposit along Coprates Catena Floor: ESP_019270_1645 ESP_019903_1645 (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
-15.1	301.	4.56	-11.5	60.5	59.0
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