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

Oxia Palus: ESP_037729_1880 ESP_037874_1880 (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
7.808	348.	-13.	8.553	57.6	56.4
Crater in Tempe Terra: ESP_037691_2170 ESP_045999_2170 (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
36.64	299.	13.0	-7.66	60.2	51.0
Channel Intersection with Aram Chaos: ESP_037782_1825 ESP_038402_1825 (Interval in Earth days: 48)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
2.655	340.	5.31	-25.6	56.2	59.7
Marte Vallis Lava: ESP_037735_1925 ESP_038012_1925 (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
12.35	182.	9.75	-6.40	55.9	58.9
Alluvial Fans in Crater: ESP_037730_1615 ESP_038007_1615 (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
-18.4	322.	6.49	-10.4	59.1	58.8
Channel within Larger Channel in Northwest Arabia Terra: ESP_037702_2160 ESP_046010_2160 (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
35.79	1.48	-5.0	-24.6	61.6	52.5
Fine-Scale Network of Valleys in Tempe Terra: ESP_037625_2255 ESP_046935_2255 (Interval in Earth days: 725)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
45.01	301.	-2.9	12.74	63.4	66.6
Light-Toned Deposits Exposed along Floor of Terra Sabaea Crater: ESP_037673_1550 ESP_038240_1550 (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
-24.8	80.8	-6.4	23.83	62.4	55.3
InSight Mission Candidate Landing Site: ESP_037829_1840 ESP_038383_1840 (Interval in Earth days: 43)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
3.983	137.	10.4	-4.64	55.9	58.2
Channelized Flow in Arimanes Rupes Region East of Mangala Valles: ESP_037734_1675 ESP_046754_1675 (Interval in Earth days: 703)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-12.2	213.	1.74	-10.3	58.0	53.1
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