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

Marte Vallis Channel between Crater Ejecta: ESP_033423_1970 ESP_033713_1970 (Interval in Earth days: 23)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
16.63	184.	-1.8	25.48	37.7	36.4
Dunes in Crater North of Antoniadi Crater: ESP_033454_2065 ESP_033955_2065 (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
26.14	57.0	1.01	22.61	39.2	37.5
Floor of Mclaughlin Crater: ESP_033391_2020 ESP_037149_2020 (Interval in Earth days: 293)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
21.90	337.	1.00	18.02	38.3	51.1
Channels and Central Pit of Terra Cimmeria Crater: ESP_033556_1435 ESP_042299_1435 (Interval in Earth days: 681)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-36.3	158.	21.1	1.451	59.8	60.1
Southern Uzboi Vallis Region: ESP_033484_1480 ESP_033629_1480 (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
-31.7	324.	10.4	23.41	56.2	57.6
Layered Light-Toned Crater-Filling Material in Northwest Hellas Region: ESP_033520_1545 ESP_033454_1545 (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
-25.2	62.0	-3.2	18.61	53.2	50.8
Shallow Crater with Fan Connected with Channel in HRSC H2938_0000_Nd3: ESP_033549_2105 ESP_033839_2105 (Interval in Earth days: 23)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
30.23	345.	-25.	-0.94	42.6	40.0
Central Ring and Pit of Mazamba Crater: ESP_033538_1520 ESP_050852_1520 (Interval in Earth days: 1349)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-27.5	290.	3.49	-20.7	54.6	49.6
Lava-Filled Crater: ESP_033635_1795 ESP_034268_1795 (Interval in Earth days: 49)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-0.32	158.	8.35	-3.45	41.0	48.0
Layer and Color Boundaries at Mawrth Vallis: ESP_033615_2030 ESP_033905_2030 (Interval in Earth days: 23)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
22.51	342.	-0.4	27.14	38.7	36.8
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