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

Aprons with Channels in Eos Chasma: ESP_064697_1665 ESP_064842_1665 (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
-13.3	317.	0.00	19.25	56.9	54.7
Miyamoto Crater: ESP_064788_1765 ESP_064854_1765 (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
-3.30	352.	1.63	-19.2	57.2	58.8
Channels with Tributaries on Rocky Plains Northwest of Argyre Region: ESP_064645_1320 ESP_082568_1320 (Interval in Earth days: 1397)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-47.5	301.	5.97	-6.62	63.9	60.6
Well-Preserved Polygons: ESP_064781_1695 ESP_065269_1695 (Interval in Earth days: 38)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-10.2	183.	4.69	-10.7	56.3	55.0
Inverted Channel in Eastern Arabia Terra: ESP_064799_1960 ESP_064522_1960 (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
15.90	49.7	-3.6	19.03	62.2	58.5
Ares Vallis: ESP_064670_1945 ESP_064815_1945 (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
14.30	331.	-1.9	16.18	60.8	60.2
4-Kilometer Rayed Crater: ESP_064513_1870 ESP_074260_1870 (Interval in Earth days: 759)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
6.696	298.	3.19	-7.81	58.0	58.9
Dunes in Becquerel Crater: ESP_064867_2020 ESP_065777_2020 (Interval in Earth days: 71)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
21.84	351.	7.65	19.56	63.9	65.0
Flow Features Associated with Well-Preserved 10-Kilometer Crater: ESP_064722_1605 ESP_065500_1605 (Interval in Earth days: 61)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-19.4	356.	-7.7	26.05	57.6	48.3
Small Cone East of Pavonis Mons: ESP_064673_1810 ESP_064818_1810 (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
1.079	250.	8.69	27.00	57.2	55.9
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