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

Possible Exposure of Polar Layered Deposits in Area Not Well Observed: ESP_023715_0910 ESP_023756_0910 (Interval in Earth days: 3)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-88.8	316.	24.2	20.11	84.0	85.5
End of Trough in South Polar Residual Cap: ESP_023504_0880 ESP_023703_0880 (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
-87.8	5.71	7.96	13.33	82.0	86.1
Gullies with Debris Aprons: ESP_023810_1395 ESP_023955_1395 (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
-40.4	196.	0.83	14.61	48.1	49.7
Well-Preserved Unnamed 6-Kilometer Diameter Crater in Daedalia Planum: ESP_023756_1600 ESP_051052_1600 (Interval in Earth days: 2127)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-19.9	227.	5.42	-8.70	35.6	47.0
Proposed Landing Site in Jezero Crater: ESP_023524_1985 ESP_023379_1985 (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
18.33	77.5	-0.5	-11.8	41.0	43.2
Auqakuh Vallis Bedform Changes: ESP_023696_2110 ESP_023762_2110 (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
30.68	60.5	-7.2	-24.5	47.5	47.9
Possible Future Landing Site Near Mounds in Chryse Region: ESP_023792_1950 ESP_024280_1950 (Interval in Earth days: 38)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
14.76	320.	1.42	-23.5	37.0	38.0
Basal Exposure of South Polar Layered Deposits: ESP_023760_1065 ESP_032542_1065 (Interval in Earth days: 685)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-73.4	132.	-5.7	9.39	73.2	72.0
Gullies with Varied Shapes on a Crater Wall: ESP_023665_1410 ESP_024087_1410 (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
-38.5	194.	6.50	-2.95	44.2	51.6
Exposure of South Polar Layered Deposits: ESP_023510_0930 ESP_040625_0930 (Interval in Earth days: 1333)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-87.1	156.	7.57	25.4	80.3	70.7
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