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

Margin of Lobate Deposit in Nereidum Montes: ESP_086272_1405 ESP_085903_1405 (Interval in Earth days: 29)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-39.4	323.	23.9	-13.2	60.4	56.6
North-Pole-Facing Deposit in Crater: ESP_086208_2275 ESP_086841_2275 (Interval in Earth days: 50)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
47.24	261.	5.23	-18.4	51.0	48.1
Features around Cerberus Palus: ESP_086252_1850 ESP_086819_1850 (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
4.904	146.	5.75	-7.57	39.5	45.0
Large Viscous Flow Feature in Nereidum Montes: ESP_086193_1370 ESP_094091_1370 (Interval in Earth days: 615)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-42.8	324.	-6.6	-14.1	63.4	48.6
Crater in Cerberus Fossae: ESP_086212_1890 ESP_086858_1890 (Interval in Earth days: 51)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
8.700	158.	4.61	25.42	38.9	41.3
North-Pole Facing Deposit in Crater: ESP_086354_2255 ESP_087000_2255 (Interval in Earth days: 50)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
45.43	237.	-7.2	12.07	49.6	44.1
Impact Monitoring in Arcadia Planitia: ESP_086330_2205 ESP_089389_2205 (Interval in Earth days: 238)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
40.34	173.	-8.4	7.166	47.3	47.9
Possible Thin Glacial Lobe in Young Crater: ESP_086309_1490 ESP_086810_1490 (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
-30.4	35.6	-7.9	3.638	56.9	63.4
A Slice through the Layercake: ESP_084979_1975 ESP_085045_1975 (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
17.49	336.	16.6	-4.34	44.6	45.3
Kasei Valles Lava: ESP_085825_1965 ESP_085614_1965 (Interval in Earth days: 16)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
16.14	285.	4.28	-6.99	39.1	40.5
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