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

Small Delta or Fan: ESP_090395_2065 ESP_082088_2065 (Interval in Earth days: 647)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
26.38	74.4	-11.	7.284	57.8	62.6
Vent East of Ascra eus Mons: ESP_090375_1925 ESP_090520_1925 (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
12.13	261.	-5.8	10.07	56.2	55.7
Terrain around Crater in Terra Sabaea: ESP_090409_2165 ESP_090132_2165 (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
36.18	50.6	-6.7	5.045	59.7	55.3
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
Morphologically Fresh Incision in Potentially Ice-Rich Mantling Deposit: ESP_090370_2225 ESP_090436_2225 (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
41.91	34.0	-3.7	-16.2	60.6	62.6
Sample of Aprons around Massifs in Erebus Montes: ESP_090404_2185 ESP_090338_2185 (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
38.34	187.	-8.8	5.02	60.5	58.4
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
Hillslope Morphologies in Roddy Crater: ESP_090307_1585 ESP_090439_1585 (Interval in Earth days: 10)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-21.2	320.	6.34	-28.5	62.5	64.4
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
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
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