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

Asimov Crater Gullies Present in MOC R1000011: ESP_039206_1320 ESP_039694_1320 (Interval in Earth days: 38)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-47.5	4.78	-5.6	-27.9	48.6	44.7
Small Cone in Hydraotes Chaos: ESP_039550_1805 ESP_039484_1805 (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
0.465	326.	-10.	11.74	51.3	50.4
USGS Dune Database Entry Number 2365-596: ESP_039514_1200 ESP_039791_1200 (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
-59.6	236.	8.44	-2.94	48.3	47.3
Candidate Landing Site for 2020 Mission in Jezero Crater: ESP_039203_1985 ESP_039348_1985 (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
18.24	77.8	-5.7	6.917	63.6	62.1
Western Wall of Crater in Kaiser Crater Dune Field: ESP_039245_1325 ESP_039944_1325 (Interval in Earth days: 54)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-47.0	18.7	4.27	-19.6	47.1	42.2
Bedform Change Detection in Aeolis Mensae: ESP_039596_1720 ESP_041086_1720 (Interval in Earth days: 116)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-7.74	151.	-0.0	18.23	46.1	32.4
Beagle 2 Lander Credible Candidate: ESP_039519_1915 ESP_040363_1915 (Interval in Earth days: 66)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
11.51	90.4	4.3	-15.9	56.9	48.4
Impact Crater into Side of Massif: ESP_039230_1545 ESP_039375_1545 (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
-25.3	66.0	-4.9	8.63	46.4	43.4
Light-Toned Deposits Exposed along Floor of Terra Sabaea Crater: ESP_039269_1550 ESP_039625_1550 (Interval in Earth days: 28)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-24.7	81.0	-4.1	6.419	45.9	40.5
Gullies: ESP_039488_1420 ESP_039343_1420 (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
-37.4	222.	5.16	-8.90	42.1	45.1
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