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

Ismenius Cavus: ESP_019333_2140 ESP_019478_2140 (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
33.77	16.9	-14.	-2.15	51.9	52.3
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
Cone Field in Phlegra Dorsa: ESP_019446_2080 ESP_019591_2080 (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
27.44	172.	-13.	0.751	52.2	52.4
Fresh 3-Kilometer Diameter Crater in Terra Sabaea: ESP_019544_1675 ESP_020177_1675 (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
-12.3	20.1	7.71	-6.37	58.0	56.7
Light-Toned Outcrops in Noctis Region: ESP_019324_1725 ESP_019469_1725 (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
-7.62	266.	-5.6	11.59	57.6	56.1
Channels and Vents in Tharsis Region: ESP_019483_2010 ESP_019549_2010 (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
20.54	241.	2.59	-17.9	50.9	53.1
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
Alpine Glacier: ESP_019213_2210 ESP_019503_2210 (Interval in Earth days: 23)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
40.86	51.3	-8.0	14.46	51.2	52.7
Abrupt Transition in Expression of North Polar Basal Stratigraphy: ESP_018898_2645 ESP_019215_2645 (Interval in Earth days: 24)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
84.25	342.	0	-13.9	65.7	70.4
Layered Terrain in Aeolis Planum: ESP_018959_1730 ESP_019025_1730 (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
-6.90	150.	4.52	-18.8	57.2	58.8
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