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

Light-Toned Bakhuysen Crater Ejecta Deposits : ESP_045957_1575 ESP_046023_1575 (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
-22.0	12.8	1.56	-21.1	59.6	60.8
Clustered Mounds with Trough-Shaped Depressions : ESP_045820_1920 ESP_055472_1920 (Interval in Earth days: 752)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
11.75	149.	1.09	19.64	47.3	51.6
Dune Forms in Viking 1 Image 436S03 : ESP_046030_1670 ESP_046452_1670 (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
-12.6	178.	4.21	-12.3	54.6	54.4
Gully Monitoring : ESP_046064_2210 ESP_052301_2210 (Interval in Earth days: 486)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
40.86	323.	2.01	-24.2	52.4	41.6
Fractures in Utopia Planitia : ESP_046138_2170 ESP_046072_2170 (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
36.42	103.	5.04	21.70	51.7	49.4
Light-Toned Material and Possible Unit Contact in Bakhuysen Crater Floor : ESP_046036_1575 ESP_046458_1575 (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
-22.3	15.5	6.93	-9.07	58.9	57.3
Light-Toned Terrain Associated with Dunes in Kaiser Crater : ESP_046181_1325 ESP_051284_1325 (Interval in Earth days: 398)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-46.9	19.2	14.6	-20.6	70.8	70.3
Candidate Impact Site Formed between September 2008 and Dec 2015 : ESP_045956_1855 ESP_064272_1855 (Interval in Earth days: 1427)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
5.372	37.3	-4.8	8.328	49.5	56.4
Impact Crater with Central Uplift : ESP_045862_2050 ESP_050688_2050 (Interval in Earth days: 376)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
24.84	80.1	7.83	-7.41	46.2	38.8
Flow Features in Argyre Region West of Hale Crater : ESP_046025_1425 ESP_046671_1420 (Interval in Earth days: 51)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-37.3	319.	-7.9	24.28	68.2	58.9
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