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

Well Preserved 7-Kilometer Diameter Impact Crater: ESP_012670_1845 ESP_011958_1845 (Interval in Earth days: 55)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
4.679	126.	4.75	-11.8	56.1	59.5
Exposure of Layered Deposits at End of Bench in Terby Crater: ESP_013516_1520 ESP_013661_1520 (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
-27.8	74.5	-7.0	8.988	37.5	35.1
Nili Fossae-NE Syrtis Phyllosilicate-Sulfate Stratigraphy: ESP_013041_1975 ESP_030025_1975 (Interval in Earth days: 1324)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
17.42	76.9	-3.2	12.81	61.2	60.4
Layered Rocks in Western Arabia: ESP_012952_2085 ESP_013941_2085 (Interval in Earth days: 77)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
28.09	344.	4.11	-9.98	68.4	59.2
Layering on Floor of Noctis Labyrinthus Pit: ESP_014076_1680 ESP_021513_1680 (Interval in Earth days: 579)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-11.8	263.	-5.4	13.21	35.2	46.5
Gullied Trough Wall: ESP_012602_1415 ESP_013881_1415 (Interval in Earth days: 100)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-38.3	188.	6.27	18.92	48.1	35.6
Pit on Crater Floor Exposing Layers: ESP_012818_1560 ESP_013174_1560 (Interval in Earth days: 28)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-23.8	50.3	-6.3	4.629	46.1	40.7
High-Latitude Gullies: ESP_013453_1075 ESP_022789_1075 (Interval in Earth days: 728)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-72.2	3.84	0.52	-16.3	54.5	58.2
Cratered Cones in Olympus Mons Aureole: ESP_013853_2130 ESP_022002_2130 (Interval in Earth days: 635)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
32.87	224.	6.20	28.86	63.2	67.7
Central Uplift of an Impact Crater in Hesperia Planum: ESP_013211_1675 ESP_013633_1675 (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
-12.4	118.	8.88	-5.92	42.9	39.0
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