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

Ridges near Vernal Crater: ESP_076737_1835 ESP_076948_1835 (Interval in Earth days: 17)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
3.400	355.	6.13	23.18	36.4	35.6
Traverse Ramp in East Coprates Chasma: ESP_076818_1640 ESP_076752_1640 (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
-15.6	306.	9.47	23.67	38.7	36.8
USGS Dune Database Entry Number 3525-631: ESP_076909_1165 ESP_076988_1165 (Interval in Earth days: 6)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-63.1	352.	-2.8	20.78	70.2	70.3
Deposits in Aeolis Dorsa: ESP_076995_1735 ESP_076784_1735 (Interval in Earth days: 16)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-6.26	154.	19.6	0.949	37.1	36.9
Downwind Hellespontus Regional Barchan Dunes: ESP_076841_1380 ESP_076221_1380 (Interval in Earth days: 48)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-41.4	44.5	-10.	12.82	53.9	43.1
Lower Interior Layered Deposits in Eastern Candor Chasma: ESP_076845_1730 ESP_076911_1730 (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
-6.94	288.	8.48	-6.96	36.9	38.6
Channels near Huygens Crater: ESP_076880_1615 ESP_077091_1615 (Interval in Earth days: 17)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-18.2	56.4	-6.7	14.11	41.6	42.9
Candidate Mud Volcanoes Targeted by Zhurong Rover: ESP_076891_2050 ESP_077023_2050 (Interval in Earth days: 10)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
24.74	109.	5.44	-19.3	43.1	44.2
Channel-Like Feature: ESP_077076_2250 ESP_077208_2250 (Interval in Earth days: 10)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
44.79	97.5	7.76	-9.81	52.7	52.5
Floor-Fractured Crater in Elysium Planitia: ESP_076810_1895 ESP_075966_1895 (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
9.398	160.	22.6	-5.00	36.2	43.3
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