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

Exhumed Light-Toned Deposit along Coprates Catena Floor: ESP_019270_1645 ESP_019903_1645 (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
-15.1	301.	4.56	-11.5	60.5	59.0
Polar Layered Deposits Unconformity: ESP_019355_2790 ESP_063517_2790 (Interval in Earth days: 3441)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
80.70	324.	-5.8	4.781	80.6	80.5
Exposure of North Polar Layered Deposits: ESP_019343_2685 ESP_028008_2685 (Interval in Earth days: 675)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
88.28	50.8	-14.	-24.3	74.8	73.1
Terrain Northwest of Hellas Planitia: ESP_019543_1465 ESP_019899_1465 (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
-33.1	50.7	0	11.96	68.5	64.4
Flow Material in Equatorial Crater: ESP_019267_1720 ESP_024858_1720 (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
-8.05	23.2	-8.4	-26.9	58.1	46.5
Pit on the Eastern Flank of Pavonis Mons: ESP_019351_1795 ESP_019984_1795 (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
-0.45	248.	-2.8	-17.6	54.7	56.1
Western Half of Crater in Sinus Sabaeus: ESP_019307_1715 ESP_019808_1715 (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
-8.50	12.3	-21.	6.908	59.3	56.0
Small Fan in Amenthes Fossae Region: ESP_019264_1895 ESP_019897_1895 (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
9.201	101.	5.29	-10.3	51.1	54.7
Excellent Megabreccia Outcrops along the Walls of Nili Fossae: ESP_019476_2005 ESP_019621_2005 (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
20.23	73.7	-7.1	8.669	51.7	51.4
Wavy Stratification Features in Crater Wall in MOC Image S14-00005: ESP_019558_1800 ESP_020125_1800 (Interval in Earth days: 44)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
0.165	357.	-10.	0.304	55.2	54.8
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