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

1-Kilometer Diameter Crater : ESP_046065_2260 ESP_046355_2260 (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
45.84	295.	-5.3	13.65	54.8	57.7
East Coprates Montes Dark Fans : ESP_045907_1665 ESP_046619_1665 (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
-13.3	297.	-2.1	12.58	55.8	52.1
Thin Layers in Eroded Crater Southwest of Bamberg Crater : ESP_046142_2165 ESP_046643_2165 (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
36.34	355.	-6.1	12.42	52.7	58.2
Light-Toned Surface in Valley in CTX Image : ESP_046011_1620 ESP_046723_1620 (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
-17.8	338.	-6.0	11.19	57.7	52.7
Layered-Target Crater : ESP_045847_2290 ESP_051042_2290 (Interval in Earth days: 405)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
48.57	127.	-3.9	23.69	52.6	47.2
Basin with Lava Fill in Southern Elysium Planitia : ESP_045938_1775 ESP_046149_1775 (Interval in Earth days: 17)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-2.57	167.	18.6	9.184	49.8	50.6
Stratigraphy of Crater Floor Materials : ESP_046035_1595 ESP_045969_1595 (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
-20.4	42.6	7.58	28.87	57.9	56.7
Light-Toned Deposits in Western Gorgonum Chaos : ESP_045977_1405 ESP_060469_1405 (Interval in Earth days: 1129)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-38.9	190.	-10.	0.139	69.8	68.6
Pasithea Dorsum : ESP_045801_1240 ESP_045867_1240 (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
-55.5	317.	2.41	-12.1	81.7	81.9
Morphologically Distinct Lyot Crater Floor : ESP_045956_2310 ESP_046233_2310 (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
50.81	29.6	4.63	-13.7	54.4	60.2
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