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

Exposures of Various North Polar Geologic Units: ESP_017845_2625 ESP_018016_2625 (Interval in Earth days: 13)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
82.42	302.	-5.5	9.318	58.6	58.2
Northern Wall of Kasei Valles: ESP_017859_2120 ESP_018492_2120 (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
31.52	297.	10.8	-7.29	41.3	45.0
Pits and Craters: ESP_017875_2305 ESP_018007_2305 (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
49.95	219.	-4.6	-28.8	43.8	46.5
Crater Floor Depressions: ESP_017934_2025 ESP_018435_2025 (Interval in Earth days: 39)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
22.32	53.1	-13.	7.638	45.4	44.9
Rampart Crater Ejecta Exposed in Cross-Section: ESP_018017_1680 ESP_026799_1680 (Interval in Earth days: 684)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-12.1	310.	-0.4	10.24	61.6	60.0
Source for Enigmatic Channel in Ceraunius Fossae: ESP_017874_2025 ESP_018296_2025 (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
22.16	248.	13.5	-0.70	43.1	45.2
Central Uplift of Impact Crater in Tyrrhena Terra: ESP_017748_1665 ESP_026108_1665 (Interval in Earth days: 651)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-13.3	93.8	8.34	24.74	61.6	57.7
Impact Crater in Northern Plains: ESP_018037_2445 ESP_018828_2445 (Interval in Earth days: 62)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
64.01	110.	7.02	25.87	48.1	51.9
Well-Preserved 10-Kilometer Diameter Impact Crater: ESP_017822_2375 ESP_018046_2375 (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
57.37	225.	-10.	14.65	46.4	44.8
Exposure of Polar Layered Deposits: ESP_017937_2680 ESP_018162_2680 (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
88.13	304.	-19.	-25.9	63.3	64.3
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