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

Landforms in Centauri Montes Region : ESP_028706_1410 ESP_028772_1410 (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
-38.5	95.7	4.18	-15.4	67.0	67.7
Crater in Utopia Planitia : ESP_028719_2290 ESP_037646_2290 (Interval in Earth days: 695)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
48.46	89.3	0	-13.9	61.7	65.9
Ravines in Melas Chasma : ESP_028633_1695 ESP_034382_1695 (Interval in Earth days: 448)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-10.1	285.	4.17	18.51	56.0	53.0
Possible Inverted Stream Channels Near Mariner Crater : ESP_028887_1430 ESP_055431_1430 (Interval in Earth days: 2068)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-36.6	193.	3.30	24.96	64.1	60.0
Pettit Crater Ejecta in Contact with Knobs and Massifs : ESP_028887_1900 ESP_042245_1900 (Interval in Earth days: 1041)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
9.773	188.	-5.0	-18.3	54.6	39.9
IR-Distinct Crater : ESP_028676_2185 ESP_054152_2185 (Interval in Earth days: 1986)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
38.06	185.	-2.3	-20.3	57.5	46.8
Well-Preserved Impact Crater : ESP_028830_2040 ESP_042043_2040 (Interval in Earth days: 1030)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
23.59	303.	-5.3	-28.5	55.9	42.2
Well-Preserved Double Crater : ESP_028631_1965 ESP_028776_1965 (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
16.16	336.	-1.4	11.21	53.0	53.0
Crater Rim Near Eumenides Dorsum : ESP_028623_1870 ESP_055510_1870 (Interval in Earth days: 2095)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
6.917	196.	-5.7	-28.8	53.5	55.4
Lava Flow Through Breached Crater Rim in Tartarus Montes : ESP_028637_2040 ESP_029072_2040 (Interval in Earth days: 34)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
23.67	172.	-8.4	27.76	54.3	55.5
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