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

Upland Valleys of Ladon Valles Basin: ESP_032073_1610 ESP_032007_1610 (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
-18.9	326.	9.50	26.89	31.5	29.8
Small Knob on South Polar Layered Deposits: ESP_032053_0920 ESP_032276_0920 (Interval in Earth days: 17)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-87.9	245.	7.08	11.94	77.4	80.0
Small Channels and Rocky Patch in Cydonia Region: ESP_031993_2115 ESP_032283_2115 (Interval in Earth days: 23)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
31.16	345.	-0.8	25.12	54.4	49.0
Jezero Crater Fan: ESP_031871_1985 ESP_031805_1985 (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
18.46	77.8	-7.2	12.84	47.1	46.8
West Coprates Chasma Dunes and Slip Face Streaks: ESP_031995_1660 ESP_031929_1660 (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
-14.0	296.	-7.5	12.92	32.5	30.9
Exposure of South Polar Layered Deposits: ESP_032092_0925 ESP_032236_0925 (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
-87.4	217.	11.3	24.85	76.4	77.7
Exposure of South Polar Layered Deposits: ESP_031779_0955 ESP_031964_0955 (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
-84.5	100.	7.93	-4.07	69.3	72.9
Crater in Elysium Planitia: ESP_031842_1865 ESP_084775_1865 (Interval in Earth days: 4125)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
6.615	150.	2.46	-7.69	39.4	42.1
Exposure of Polar Layered Deposits Not Observed by MGS: ESP_031920_0915 ESP_031879_0915 (Interval in Earth days: 3)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-88.4	268.	14.8	22.22	74.9	73.3
Light-Toned Layered Material Exposed in Coprates Chasma Scarp Wall: ESP_031942_1645 ESP_032575_1645 (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
-15.2	303.	-3.3	-25.0	32.1	37.0
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