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

Potential Mars Landing Site near Mounds Associated with Crater Rim: ESP_021919_2135 ESP_021642_2135 (Interval in Earth days: 22)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
32.97	336.	-23.	-0.04	71.4	71.0
Victoria Crater: ESP_021747_1780 ESP_022380_1780 (Interval in Earth days: 49)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-2.04	354.	-2.8	-23.0	49.2	43.5
Ridges around Crater Rim Valley in Terra Cimmeria: ESP_021901_1395 ESP_021756_1395 (Interval in Earth days: 12)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-40.3	113.	9.90	-3.69	39.8	42.6
Kaiser Crater Dune Gullies: ESP_021720_1330 ESP_020876_1330 (Interval in Earth days: 65)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-46.7	20.1	-22.	3.645	46.0	56.9
Impact Crater with Central Uplift: ESP_021998_1610 ESP_022420_1610 (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
-18.8	344.	-5.5	-20.5	40.2	36.6
Well-Preserved 5-Kilometer Diameter Impact Crater: ESP_021767_1315 ESP_022400_1315 (Interval in Earth days: 49)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-48.2	173.	6.74	-8.25	43.6	40.1
Layers in Noctis Region Pit: ESP_021869_1690 ESP_030704_1690 (Interval in Earth days: 688)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-10.8	264.	2.83	-14.7	43.7	44.8
Many Small Cones in Amazonis Planitia: ESP_021990_1985 ESP_022412_1990 (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
18.78	198.	-4.5	-18.4	59.5	56.0
Impact Crater into Heavily Mantled Pole-Facing Slope: ESP_021771_1505 ESP_021626_1505 (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
-29.2	63.2	-8.3	-19.5	41.9	44.7
Well-Preserved Flow-Ejecta Crater East of Juventae Chasma: ESP_021683_1735 ESP_057933_1740 (Interval in Earth days: 2824)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-6.25	301.	5.27	14.08	47.4	34.0
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