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

Planned ExoMars Landing Site in Oxia Planum: ESP_083252_1980 ESP_083107_1980 (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
17.59	335.	-6.0	-19.8	64.2	65.6
Fresh Crater near Ice-Rich Terrain: ESP_083188_1295 ESP_083254_1295 (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
-50.3	290.	7.09	-8.45	50.5	50.7
Hellas Planitia: ESP_082906_1370 ESP_082972_1370 (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
-42.7	70.5	-5.0	-23.5	54.0	54.5
Flow Features on Ice-Rich Plateau on Malea Patera: ESP_083276_1165 ESP_083144_1165 (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
-63.1	53.5	-7.0	15.29	55.0	55.2
Crater: ESP_083271_1585 ESP_083772_1585 (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
-21.2	181.	0	13.72	47.8	40.5
Channel Entering Crater: ESP_082956_1395 ESP_083378_1395 (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
-40.3	143.	4.73	-7.28	51.9	46.6
Hillslope Morphologies in Crater: ESP_082945_1510 ESP_083011_1510 (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
-28.8	83.4	-4.8	-26.4	51.8	52.7
Juventae Chasma Interior Deposit Layers: ESP_082937_1760 ESP_082357_1760 (Interval in Earth days: 45)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-4.16	297.	8.05	-7.44	54.7	58.4
Ariadnes Colles: ESP_083100_1450 ESP_083588_1450 (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
-34.6	171.	3.68	-22.4	49.2	44.5
Channels in Tyrrhena Terra: ESP_083116_1520 ESP_083327_1520 (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
-27.6	93.9	0.05	-5.04	49.2	46.7
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