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

Potential Landing Sites in Capri Chasma: ESP_090426_1665 ESP_090070_1665 (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
-13.4	311.	4.49	-21.8	59.4	62.7
Bench in Samara Valles: ESP_090425_1545 ESP_090715_1545 (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
-25.0	340.	3.09	12.71	63.4	60.4
Flow Obstacle in Lobate Debris Apron: ESP_090608_2215 ESP_090107_2215 (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
40.89	11.8	27.4	9.221	61.0	55.7
Monitor Changes in Intracrater Mounds: ESP_090444_2195 ESP_090378_2195 (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
39.18	175.	-8.2	5.181	61.3	59.2
Layered Mound near Mawrth Vallis: ESP_090359_2045 ESP_090425_2045 (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
24.02	335.	8.76	-7.68	55.6	57.6
Okavango Valles: ESP_090595_2185 ESP_090516_2185 (Interval in Earth days: 6)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
38.24	8.82	17.2	-4.81	60.9	61.7
Survey of Terrain around Ice-Exposing Crater: ESP_090417_2195 ESP_090628_2195 (Interval in Earth days: 17)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
39.25	190.	8.58	-5.83	59.5	63.6
Kasei Valles Dissected Alluvial Fans: ESP_090400_2060 ESP_090466_2060 (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
25.88	297.	-0.8	-16.8	57.0	59.0
Inverted Dendritic Channels in Noachis Terra Crater: ESP_090370_1555 ESP_090581_1555 (Interval in Earth days: 17)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-24.1	41.6	6.89	-5.62	63.2	62.6
Alluvial Fan in Coprates Catena Trough: ESP_090308_1650 ESP_090453_1650 (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
-14.6	294.	-16.	8.504	61.8	59.4
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