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

Fluvial Features in Noachis Terra: ESP_086350_1580 ESP_086772_1580 (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
-21.5	353.	6.39	-17.1	51.1	58.3
Gully and Lobate Glacier Fill of Fresh Looking Crater: ESP_086259_2175 ESP_086826_2175 (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
37.33	311.	2.92	-6.63	45.5	43.8
Young Impact on Layers in Protonilus Mensae: ESP_086295_2230 ESP_086717_2230 (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
42.61	46.9	5.28	-12.4	47.7	46.4
Thermophysical Boundary West of Hebrus Valles: ESP_086345_2015 ESP_087123_2015 (Interval in Earth days: 60)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
21.09	124.	5.18	-9.06	39.9	43.0
Possible Thin Glacial Lobe in Young Crater: ESP_086309_1490 ESP_086810_1490 (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
-30.4	35.6	-7.9	3.638	56.9	63.4
Light-Toned Exposures in Capri Chasma: ESP_086246_1670 ESP_086312_1670 (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
-13.0	312.	9.05	-17.0	45.0	47.7
Lethe Vallis Chevron Shaped Landforms: ESP_086344_1840 ESP_086845_1840 (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
4.028	155.	-7.9	5.786	41.4	44.5
Head of Lethe Vallis: ESP_086199_1840 ESP_087056_1840 (Interval in Earth days: 67)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
3.785	153.	5.44	20.19	39.3	45.1
Impact Monitoring in Arcadia Planitia: ESP_086330_2205 ESP_089389_2205 (Interval in Earth days: 238)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
40.34	173.	-8.4	7.166	47.3	47.9
Deuteronilus Mensae: ESP_086256_2255 ESP_085676_2255 (Interval in Earth days: 45)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
45.16	28.6	25.3	-1.94	47.9	56.0
	Page 40 of 881 (8,805 images)