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

Mounds in Oxia Colles: ESP_064604_1985 ESP_064459_1985 (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
18.44	331.	8.61	-7.88	60.7	60.8
Sinuous Ridge Feature in CTX D21_035468_1545_XN_25S202W: ESP_064716_1535 ESP_047534_1535 (Interval in Earth days: 1339)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-26.2	158.	26.4	2.235	55.6	47.5
Channel: ESP_064748_1765 ESP_065724_1765 (Interval in Earth days: 76)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-3.41	3.86	3.24	-8.49	57.1	53.8
Blocky Terrain in Elysium Planitia: ESP_064835_1830 ESP_090432_1830 (Interval in Earth days: 1994)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
3.193	147.	5.27	-16.6	58.1	57.9
Baetis Chasma and nearby Impact Crater: ESP_064711_1750 ESP_072625_1750 (Interval in Earth days: 617)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-4.75	294.	-5.6	5.692	57.7	57.5
Aprons with Channels in Eos Chasma: ESP_064697_1665 ESP_064842_1665 (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
-13.3	317.	0.00	19.25	56.9	54.7
Valleys in Central Pit of Crater: ESP_064630_1525 ESP_073599_1525 (Interval in Earth days: 699)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-27.4	347.	8.33	-13.2	58.2	58.2
Transition from Channel to Ridge: ESP_064841_1565 ESP_065751_1565 (Interval in Earth days: 71)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-23.4	348.	-6.5	5.135	56.9	46.6
Miyamoto Crater: ESP_064788_1765 ESP_064854_1765 (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
-3.30	352.	1.63	-19.2	57.2	58.8
Well-Preserved Polygons: ESP_064781_1695 ESP_065269_1695 (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
-10.2	183.	4.69	-10.7	56.3	55.0
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