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

Possible Blocky Deposit in Melas Chasma: ESP_013508_1665 ESP_014141_1665 (Interval in Earth days: 49)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-13.2	289.	6.08	-18.0	39.2	35.6
Gullies Previously Identified in MOC Image: ESP_013849_1080 ESP_013981_1080 (Interval in Earth days: 10)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-71.9	354.	-7.6	-22.1	56.8	59.0
Light-Toned Material in a Crater in Iani Chaos: ESP_013572_1795 ESP_022710_1795 (Interval in Earth days: 712)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-0.54	341.	-3.2	13.82	44.7	37.9
Crater in the Sirenum Fossae Region: ESP_012918_1450 ESP_013340_1450 (Interval in Earth days: 32)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-34.4	201.	-7.6	-20.0	44.4	40.3
Basal Exposure of South Polar Layered Deposits: ESP_013145_1070 ESP_013277_1070 (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
-73.0	133.	0.46	-14.5	55.6	56.1
South Polar Layered Deposits Exposed in Bend in Trough Wall: ESP_013830_0940 ESP_014027_0940 (Interval in Earth days: 15)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-85.7	172.	7.85	26.64	66.5	67.5
Exposure of Thick Layered Deposits in Hebes Chasma: ESP_013205_1790 ESP_021565_1790 (Interval in Earth days: 651)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-0.82	283.	-25.	-3.43	50.5	51.4
Eastern Tooting Crater Impact Processes: ESP_013735_2035 ESP_014157_2035 (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
23.18	207.	6.42	-8.32	57.4	52.6
Central Structure of a Large Impact Crater: ESP_013134_1610 ESP_021494_1610 (Interval in Earth days: 652)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-18.6	62.6	-6.3	14.94	43.1	44.9
Well-Preserved 12 Kilometer Impact Crater on East Rim in Isidis Region: ESP_014016_1945 ESP_022376_1945 (Interval in Earth days: 652)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
14.52	98.4	-8.6	14.23	48.5	51.5
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