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

Volcanic Vent Southeast of Pavonis Mons: ESP_086802_1790 ESP_087079_1790 (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
-1.03	249.	8.99	-22.0	45.9	50.7
Layers and Features in Arabia Terra Crater: ESP_087100_1860 ESP_087667_1860 (Interval in Earth days: 44)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
6.225	34.5	-6.5	7.77	46.6	49.1
Small Mesa: ESP_087081_2175 ESP_087015_2175 (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
37.39	189.	-8.7	7.839	43.5	42.2
Arabia Terra: ESP_086877_1880 ESP_087510_1880 (Interval in Earth days: 50)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
8.404	1.37	6.07	-6.74	43.3	48.4
North-Pole-Facing Deposit in Crater Associated with Headwall Erosion: ESP_087078_2245 ESP_087144_2245 (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
44.13	268.	3.97	-10.9	44.1	45.1
Concentric Crater Fill: ESP_087124_2205 ESP_087190_2205 (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
40.20	93.4	5.73	-9.98	42.7	43.9
Ridge Over Hill in Hellas Planitia: ESP_086821_1375 ESP_086676_1375 (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
-41.9	97.7	-3.9	-15.1	72.1	70.7
Small Alluvial Fans in Kasei Valles: ESP_087156_2065 ESP_087011_2065 (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
26.44	299.	26.2	13.41	39.5	40.5
Hillslope Morphologies near Murray Crater: ESP_087074_1555 ESP_087219_1555 (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
-24.0	28.1	-7.1	10.08	63.0	63.5
Fluvial Deposit in Noachis Terra: ESP_087181_1560 ESP_087893_1560 (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
-23.5	346.	-8.2	22.88	63.9	67.5
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