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

Extra-Crater Sinuous Ridge: ESP_074491_1905 ESP_075269_1905 (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
10.54	110.	-0.7	-23.8	59.2	53.5
Channel Head in Newton Crater: ESP_074356_1405 ESP_074923_1405 (Interval in Earth days: 44)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-38.9	202.	-2.9	-17.9	48.7	42.6
Small Delta or Fan: ESP_074435_1465 ESP_075292_1465 (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
-33.2	205.	-7.5	6.888	47.4	36.9
Light-Toned Deposits in Iani Chaos: ESP_074443_1790 ESP_074377_1790 (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
-0.76	341.	6.66	27.24	53.4	52.3
Pole-Facing Gullies in 7-Kilometer Crater within Bond Crater: ESP_074457_1470 ESP_074747_1470 (Interval in Earth days: 22)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-32.7	323.	1.02	17.64	46.5	41.4
Highest Point of Olympus Mons: ESP_074223_1975 ESP_074368_1975 (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
17.32	226.	-8.1	6.665	64.2	63.1
Small Delta or Fan: ESP_073960_1630 ESP_074105_1630 (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
-16.6	211.	-5.2	10.88	53.8	51.2
Well-Preserved 3-Km Impact Crater in Nereidum Montes: ESP_074035_1360 ESP_073890_1360 (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
-43.6	326.	11.5	-7.18	53.3	56.9
Northeast Syrtis Major Dune Field: ESP_074202_2005 ESP_083169_2005 (Interval in Earth days: 698)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
20.27	78.9	2.83	20.28	65.1	64.2
Lava-Crater Interaction in Elysium Planitia: ESP_073949_1860 ESP_074239_1860 (Interval in Earth days: 23)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
5.812	148.	-1.0	25.38	58.9	56.1
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