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

Dune Change Detection in Kaiser Crater: ESP_022221_1330 ESP_022300_1330 (Interval in Earth days: 7)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-46.7	20.1	-4.9	22.31	39.9	37.5
Linear Gully in Hellas Basin Region: ESP_022074_1315 ESP_022931_1315 (Interval in Earth days: 67)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-48.3	73.7	-1.3	18.17	41.3	40.5
Polar Cap Monitoring Site: ESP_022145_0940 ESP_022131_0940 (Interval in Earth days: 2)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-86.0	350.	-7.7	6.508	65.3	63.8
Possible MSL Rover Landing Site in Crater Floor with Layered Mesa: ESP_022180_1515 ESP_022246_1515 (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
-28.2	56.8	-5.5	-26.2	36.8	37.9
Gully Monitoring Site: ESP_022108_1410 ESP_022385_1410 (Interval in Earth days: 21)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-38.8	223.	0.66	-26.4	38.0	38.2
Small Mounds in Chryse Planitia: ESP_022025_2000 ESP_040328_2000 (Interval in Earth days: 1426)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
19.72	322.	-4.4	12.17	59.9	52.7
Polar Cap Monitoring Site: ESP_022210_0930 ESP_022064_0930 (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
-86.7	16.1	-1.1	13.12	65.4	63.8
Dune Features: ESP_022181_1345 ESP_023025_1345 (Interval in Earth days: 66)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-45.1	28.8	23.5	0.924	37.4	40.5
Western Rim of Very Well-Preserved Impact Crater: ESP_022291_1995 ESP_022713_1995 (Interval in Earth days: 33)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
19.26	259.	-3.5	-14.7	56.8	52.2
Possible Source Region of Harris Crater Fan: ESP_022140_1585 ESP_021784_1585 (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
-21.4	67.2	3.34	-9.00	37.3	42.6
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