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

Crater within a Crater in the Nilosyrtis Mensae Region: ESP_017063_2155 ESP_018276_2155 (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
35.15	71.4	-10.	13.25	41.8	42.0
Coprates Chasma Wall: ESP_017200_1680 ESP_017912_1680 (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
-11.7	296.	-9.0	1.653	59.3	61.1
Rocky Hill: ESP_016922_1615 ESP_017423_1615 (Interval in Earth days: 39)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-18.5	326.	5.41	22.56	61.0	63.1
Distal Edge of Flow from Galaxias Fossae: ESP_017179_2175 ESP_017245_2175 (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
37.16	142.	6.93	-10.3	40.5	42.0
Heart-Shaped Pit in Acheron Catena Seen in MOC M02-01153: ESP_016977_2165 ESP_017755_2165 (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
36.22	258.	-2.6	-13.7	41.1	42.8
Well-Preserved Mid-Latitude Crater: ESP_016981_2210 ESP_017482_2210 (Interval in Earth days: 39)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
40.75	149.	-6.3	6.555	42.1	40.9
Intersecting Graben in Ulysses Fossae: ESP_017268_1915 ESP_017413_1915 (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
11.38	237.	-11.	3.258	47.2	46.7
Central Structure and Layered Bedrock in 25-Kilometer Diameter Crater: ESP_017002_1535 ESP_017147_1535 (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
-26.0	303.	-3.1	10.15	67.4	67.7
Well-Preserved Impact Crater: ESP_017119_1635 ESP_025756_1635 (Interval in Earth days: 673)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-16.3	347.	2.14	-18.7	61.2	60.0
Central Uplift of an Impact Crater: ESP_017181_1735 ESP_024829_1735 (Interval in Earth days: 596)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-6.23	93.6	4.73	-14.2	54.9	44.3
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