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

Central Mound of Crater in Tyrrhena Terra: ESP_042934_1690 ESP_043356_1690 (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
-10.6	98.2	-5.6	-19.9	51.7	56.1
Light-Toned Layered Material along Ius Chasma Plateau: ESP_042822_1715 ESP_043534_1715 (Interval in Earth days: 55)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-8.21	275.	-0.0	18.35	48.9	53.2
Double-Terrace Crater in Arcadia Planitia: ESP_043036_2275 ESP_043102_2275 (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
47.23	183.	16.5	2.794	42.2	43.0
Coprates Region Falling Dunes and Landslide Scarps: ESP_043098_1650 ESP_043599_1650 (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
-15.0	303.	-25.	1.007	57.2	59.1
Steep Slopes in Melas Chasma: ESP_043072_1685 ESP_043573_1685 (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
-11.3	290.	-7.9	19.28	53.5	55.3
Central Melas Chasma Floor: ESP_042927_1680 ESP_045749_1680 (Interval in Earth days: 220)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-11.7	288.	-0.0	20.23	51.9	53.9
Landforms in Lyot Crater: ESP_043068_2295 ESP_043358_2295 (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
48.94	30.1	8.61	25.50	43.4	40.5
Galaxias Fossae: ESP_043064_2180 ESP_043565_2180 (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
37.43	142.	0	19.09	40.5	37.9
Crater Floor Deposits: ESP_043080_2045 ESP_051150_2045 (Interval in Earth days: 629)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
24.04	67.5	-1.1	-17.0	39.6	38.2
Flow-Like Features Near Kasei Valles: ESP_043085_2070 ESP_043797_2070 (Interval in Earth days: 56)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
26.95	290.	4.74	24.01	39.0	37.9
	Page 415 of 896 (8,955 images)