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

Streamlined Form and Channel Floor in Athabasca Valles: ESP_011825_1895 ESP_012814_1895 (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
9.439	156.	-3.5	-16.8	59.8	59.0
Emission of Dark Material in Cerberus Fossae: ESP_011785_1875 ESP_011930_1875 (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
7.411	168.	-8.3	7.691	59.6	58.6
Layered Bedrock Exposures in Massif North of Hellas Basin: ESP_011683_1540 ESP_012395_1540 (Interval in Earth days: 56)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-25.6	77.4	-4.3	16.97	59.2	49.7
Possible Pingos on Floor of Small Craters: ESP_011675_1470 ESP_015987_1470 (Interval in Earth days: 336)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-32.5	296.	-6.2	-21.4	61.0	61.2
Gullied Pit: ESP_012491_1170 ESP_012992_1170 (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
-62.5	344.	-2.8	8.87	57.6	50.2
Channel Cut into Fan in Eos Chasma in MOC R06-01376: ESP_011806_1665 ESP_020021_1665 (Interval in Earth days: 640)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-13.2	317.	-3.9	10.24	57.1	56.2
Unnamed Channel Reach East of Juventae Chasma: ESP_011701_1790 ESP_012334_1790 (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
-0.97	302.	1.8	-15.9	57.4	57.2
Layers in Valley on the West Flank of Arsia Mons: ESP_011743_1725 ESP_011809_1725 (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
-7.58	236.	6.94	-16.1	56.6	58.2
Knobs in East Candor Chasma: ESP_012031_1720 ESP_012664_1720 (Interval in Earth days: 50)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-8.03	294.	-7.5	-28.0	56.4	53.4
Rayed 6-Kilometer Diameter Crater: ESP_011893_1635 ESP_012315_1635 (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
-16.3	102.	-3.5	-15.7	56.5	53.8
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