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

Dunes Dubbed Hazar: ESP_062627_2555 ESP_054029_2555 (Interval in Earth days: 670)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
75.24	293.	7.72	-8.08	56.3	58.9
Layered Material and Wall Spur in East Candor Chasma: ESP_062852_1725 ESP_069408_1725 (Interval in Earth days: 511)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-7.27	289.	4.20	-7.91	57.8	58.4
The Life of a Glacier on Mars: PSP_008809_2215 PSP_009455_2215 (Interval in Earth days: 51)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
41.27	54.7	-6.7	10.01	42.9	43.4
An Impact North of Valles Marineris: ESP_011425_1775 ESP_012282_1775 (Interval in Earth days: 67)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-2.35	278.	-7.2	29.98	58.0	53.4
Central Peak of a Large Crater: ESP_014361_1585 ESP_021587_1585 (Interval in Earth days: 563)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-21.5	44.7	-14.	6.137	35.0	43.9
A Possible Landing Region for a Future Mars Sample Return: ESP_062886_1990 ESP_063308_1990 (Interval in Earth days: 33)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
18.66	77.1	11.5	-14.3	46.8	51.5
Barchan Dune Source: ESP_062861_2650 ESP_062796_2650 (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
84.90	332.	18.5	5.525	64.7	64.0
Mounds Cut by a Fissure: ESP_062943_2230 ESP_062877_2230 (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
42.80	319.	-8.8	8.21	48.2	46.1
Sibiti Crater: ESP_062364_1675 ESP_062575_1675 (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
-12.3	294.	5.62	-11.1	60.8	61.9
Undulations on Dokka Crater Ice Dome: ESP_062353_2570 ESP_062406_2570 (Interval in Earth days: 4)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
77.05	213.	4.78	-11.2	55.7	57.1
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