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

Scalloped Features in Deuteronilus Mensae: ESP_016313_2265 ESP_016590_2265 (Interval in Earth days: 22)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
46.17	23.3	8.14	-8.96	44.5	44.6
Crater with Lineated Material on Floor: ESP_016824_1465 ESP_016969_1465 (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
-33.2	124.	-2.9	10.86	71.0	71.5
Isolated Layered Mound in Trough Between Layered Benches in Terby Crater: ESP_016628_1520 ESP_016773_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
-27.6	74.4	0.18	16.62	64.9	65.4
Columnar Jointing in West Wall of Crater in Marte Vallis: ESP_016360_2020 ESP_016505_2020 (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
21.55	184.	7.23	21.49	39.4	38.5
25-Kilometer Diameter Gullied Impact Crater in Acidalia Planitia: ESP_016592_2170 ESP_016737_2170 (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
36.54	329.	-3.7	9.38	41.6	40.3
Very Well-Preserved 12-Kilometer Diameter Crater: ESP_016569_2320 ESP_016846_2320 (Interval in Earth days: 22)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
51.40	234.	-1.5	-15.9	46.0	46.1
Possible Phyllosilicate-Rich Area in Syrtis Major: ESP_016628_2040 ESP_017340_2040 (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
23.69	68.6	-7.2	6.233	41.2	42.0
Fretted Valley Outlet: ESP_016391_2195 ESP_016668_2195 (Interval in Earth days: 22)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
38.96	56.1	-0.8	-19.4	42.2	43.3
Wrinkle Ridges in Hesperia Planum: ESP_016455_1535 ESP_016811_1535 (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
-26.2	117.	-5.9	7.118	62.1	65.3
Light-Toned Layering in Hebes Mensa: ESP_016462_1785 ESP_016818_1785 (Interval in Earth days: 27)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-1.35	282.	0.48	14.17	47.0	49.0
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