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

Layering in Rutherford Crater: ESP_066938_1990 ESP_067070_1990 (Interval in Earth days: 10)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
18.94	349.	-0.3	-20.9	53.4	53.2
Gullied Slope: ESP_067136_1115 ESP_066991_1115 (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
-68.4	1.64	-1.9	-17.9	59.4	58.6
Pasted-on Material on Crater Ejecta: ESP_067006_1855 ESP_057986_1855 (Interval in Earth days: 703)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
5.595	295.	3.93	-6.11	44.6	41.1
Gully Monitoring and Topography: ESP_067155_1415 ESP_074132_1415 (Interval in Earth days: 543)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-38.3	195.	5.52	26.12	41.5	49.6
Flow-Like Feature within Adamas Labyrinthus: ESP_067290_2195 ESP_067422_2195 (Interval in Earth days: 10)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
39.14	101.	7.82	-6.03	62.5	61.6
Channel in Margaritifer Terra: ESP_066965_1680 ESP_067783_1680 (Interval in Earth days: 64)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-12.0	336.	-0.0	13.94	38.6	39.3
Lobate Apron in Phlegra Montes: ESP_067169_2165 ESP_067301_2165 (Interval in Earth days: 10)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
36.01	164.	0.39	-14.9	62.3	61.5
Spider Terrain: ESP_066936_0930 ESP_066963_0930 (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
-86.8	86.2	14.5	4.628	69.8	71.1
Gullies Emanating from Lobate Flow: ESP_067296_1315 ESP_058856_1315 (Interval in Earth days: 658)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-48.0	309.	9.71	-12.4	47.6	50.0
Xanthe Dorsa: ESP_066965_2140 ESP_067176_2140 (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
33.69	331.	-5.3	17.45	63.6	59.5
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