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

Small Volcano in Northern Syria Planum: ESP_016318_1710 ESP_016951_1710 (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
-8.76	254.	6.70	-9.92	48.9	55.9
Large-Scale Slumping in Moreux Crater: ESP_016642_2215 ESP_017710_2215 (Interval in Earth days: 83)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
41.13	44.1	-7.3	6.121	42.8	41.2
Crater within Schiaparelli Crater Filled with Layered Rock: ESP_016406_1790 ESP_017118_1790 (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
-0.93	13.8	-24.	-5.60	48.3	52.2
Pits along the Claritas Rupes: ESP_016450_1570 ESP_016516_1570 (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
-22.5	252.	7.58	-14.9	58.8	60.8
Candidate MSL Landing Site in Northeast Syrtis Major: ESP_016720_1980 ESP_016786_1980 (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
17.78	76.9	2.08	-17.9	41.7	43.6
Fresh 6-Kilometer Diameter Crater South of Coprates Chasma: ESP_016422_1625 ESP_017345_1625 (Interval in Earth days: 72)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-17.1	296.	-0.6	9.867	55.4	62.6
Light-Toned Layering in Coprates Catena Trough: ESP_016857_1645 ESP_017569_1645 (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
-15.1	301.	0	9.274	58.6	62.2
Relatively Fresh Crater Cut by Erosion: ESP_016738_1730 ESP_019296_1730 (Interval in Earth days: 200)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-7.05	309.	-7.3	16.52	53.0	55.8
Gullied Crater Wall: ESP_016343_2350 ESP_017978_2350 (Interval in Earth days: 128)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
54.87	284.	-3.8	7.591	49.3	44.4
Well-Preserved 30-Kilometer Diameter Impact Crater with Bedrock Exposures: ESP_016760_1585 ESP_017538_1585 (Interval in Earth days: 61)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-21.4	70.1	-2.0	-13.5	62.0	67.8
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