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

Well-Preserved 4-Kilometer Impact Crater: ESP_083095_1535 ESP_083240_1535 (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
-26.2	307.	-5.3	9.499	49.9	46.9
Inverted Channel in Arabia Terra: ESP_083014_1895 ESP_083370_1895 (Interval in Earth days: 28)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
9.391	354.	-5.5	4.297	60.7	58.2
Streamlined Features in Argyre Planitia: ESP_083108_1320 ESP_083042_1320 (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
-47.5	316.	-9.5	8.121	52.2	51.9
Landslide in Crater in Arabia Terra: ESP_082935_1940 ESP_082869_1940 (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
13.68	350.	-0.2	23.3	62.5	60.7
Gullied Crater: ESP_083220_1425 ESP_083576_1425 (Interval in Earth days: 28)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-37.0	136.	-2.3	12.65	48.1	42.2
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
Hebes Chasma Layered Deposits: ESP_083043_1790 ESP_083188_1790 (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
-0.77	283.	6.50	20.00	55.3	53.4
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
Large Gully: ESP_083213_1425 ESP_083358_1425 (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
-37.1	329.	-22.	-7.36	49.9	46.6
Planned ExoMars Landing Site in Oxia Planum: ESP_083041_1980 ESP_082975_1980 (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
17.80	335.	2.09	23.42	64.3	62.7
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