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

Gullied Crater Wall: ESP_020355_1385 ESP_020856_1385 (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
-41.0	203.	0.96	20.15	63.0	54.2
Channels and Lava Flows: ESP_020261_2010 ESP_020683_2010 (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
20.66	241.	6.17	-9.72	57.1	61.6
Ridges in Schiaparelli Crater: ESP_020322_1785 ESP_020955_1785 (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
-1.36	18.1	15.4	-6.19	53.7	54.7
Spiders in Variety of Terrains: ESP_020229_0930 ESP_020230_0930 (Interval in Earth days: 0)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-87.0	86.4	9.23	-2.36	88.6	89.9
Valleys in Arabia Terra: ESP_020203_2180 ESP_026994_2180 (Interval in Earth days: 529)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
37.49	24.1	-6.7	-24.4	62.9	44.3
A Potential Future Mars Landing Site: Mounds in Acidalia Planitia: ESP_017950_2205 ESP_018583_2205 (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
40.06	333.	-5.1	-19.3	42.7	46.8
Proposed Future Mars Landing Site: Acidalia Planitia Mud Volcanoes: ESP_019612_2250 ESP_025203_2250 (Interval in Earth days: 436)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
44.51	317.	-3.1	-17.0	56.8	44.5
Fresh 12-Kilometer Diameter Crater in Amenthes Planum: ESP_019699_1845 ESP_019277_1845 (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
4.574	106.	3.31	14.79	53.4	51.6
Dunes: ESP_019952_1380 ESP_029064_1380 (Interval in Earth days: 710)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-41.5	45.5	6.44	-26.8	68.0	66.4
Aganippe Fossa: ESP_019879_1695 ESP_019945_1695 (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
-10.5	234.	5.1	-17.5	56.5	58.0
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