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

Melas Chasma: ESP_076489_1675 ESP_076977_1675 (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
-12.2	286.	0	15.90	35.7	38.9
Crater in Arabia Terra: ESP_076631_2175 ESP_077462_2175 (Interval in Earth days: 65)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
37.29	5.51	-8.7	7.098	53.9	45.4
Stepped Fan on West Crater Wall of Gale Crater: ESP_076534_1750 ESP_077154_1750 (Interval in Earth days: 49)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-5.00	136.	8.87	-1.44	35.0	40.0
Collapse Terrain near Orson Welles Crater: ESP_076699_1780 ESP_084545_1780 (Interval in Earth days: 612)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-1.83	313.	0.97	-21.6	36.3	41.3
Pitted Mounds in Chryse Planitia: ESP_076606_2230 ESP_077292_2230 (Interval in Earth days: 53)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
42.89	326.	-0.9	-13.6	57.6	51.0
Channels in Flaugergues Crater: ESP_076578_1620 ESP_076921_1620 (Interval in Earth days: 27)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-17.9	18.1	0.55	-14.7	37.6	42.6
Inverted Channel and Possible Lake Deposits: ESP_076462_1725 ESP_084242_1725 (Interval in Earth days: 606)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-7.56	303.	-5.5	29.60	35.8	38.1
Crater in Crater Exposing Bedrock: ESP_076436_1560 ESP_076858_1560 (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
-23.5	294.	-2.3	24.42	38.2	41.4
Streamlined Hills in Osuga Valles: ESP_076435_1640 ESP_076369_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
-16.0	320.	5.27	22.25	35.6	33.7
Youthful Crater in THEMIS V22898007 and at Edge of MOC E11-03928: ESP_076415_1345 ESP_084037_1345 (Interval in Earth days: 594)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-45.2	150.	5.97	-6.29	48.5	41.2
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