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

Crater-Edge Mound in Chryse Planitia: ESP_081617_2055 ESP_073441_2055 (Interval in Earth days: 637)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
25.41	334.	-18.	-8.07	59.8	64.5
Small Gullies on Ridge and Lobate Flows on Crater Floor: ESP_081539_1360 ESP_081882_1360 (Interval in Earth days: 27)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-43.7	309.	13.8	-16.5	72.5	70.3
Streamlined Landforms adjacent to Shalbatana Vallis: ESP_081512_1890 ESP_080800_1890 (Interval in Earth days: 55)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
8.966	318.	28.8	14.43	54.2	53.2
Dune Monitoring in Northern Mid-Latitude Crater: ESP_081456_2340 ESP_089763_2340 (Interval in Earth days: 647)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
53.71	41.5	8.54	-0.90	62.9	55.6
Aeolis Dorsa Branching Fluvial Deposits: ESP_081439_1735 ESP_081584_1735 (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
-6.30	154.	9.46	27.06	58.5	56.8
Fresh Crater in Southern Mid-Latitudes: ESP_081572_1380 ESP_090169_1380 (Interval in Earth days: 670)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-41.4	129.	-4.5	15.50	72.2	72.6
Curving Ridges in Aeolis Planum: ESP_079382_1735 ESP_080081_1735 (Interval in Earth days: 55)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-6.26	151.	-2.2	-21.0	59.7	62.1
A Sedimentary Fan in Southeast Gale Crater: ESP_079699_1740 ESP_079844_1740 (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
-5.80	138.	-12.	9.278	60.9	59.6
Crater in Arabia Terra: ESP_080864_2145 ESP_080363_2145 (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
34.04	7.53	10.5	-7.04	50.7	48.5
Topography of Rim Mesas near Scandia Colles: ESP_080962_2530 ESP_080975_2530 (Interval in Earth days: 1)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
72.82	205.	-7.9	7.705	64.8	63.8
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