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

Rise in Eastern Echus Chasma: ESP_037771_1870 ESP_046092_1870 (Interval in Earth days: 648)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
7.121	282.	-12.	17.04	57.6	47.8
Boulders inside of Pits on a Mesa: ESP_037747_1810 ESP_073986_1810 (Interval in Earth days: 2824)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
1.014	217.	-6.3	20.01	57.1	55.5
Meridiani Planum Stratigraphy: ESP_037847_1805 ESP_038401_1805 (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
0.330	6.52	9.92	-3.02	56.0	57.3
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
Lobate Flow Feature: ESP_037714_1435 ESP_037648_1435 (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
-36.2	42.0	6.49	23.10	65.3	64.8
Light-Toned Deposits in Noctis Labyrinthus: ESP_037732_1740 ESP_046752_1740 (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
-6.06	267.	2.13	-10.1	57.0	52.5
Herschel Crater Dunes Change Detection: ESP_037948_1645 ESP_038291_1645 (Interval in Earth days: 27)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-15.1	131.	3.51	-24.6	57.5	58.0
Ritchey Crater Central Uplift: ESP_037691_1515 ESP_037968_1515 (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
-28.4	308.	6.08	-10.2	62.6	61.3
Well-Preserved Impact Crater Near Meroe Patera: ESP_037726_1870 ESP_046179_1870 (Interval in Earth days: 658)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
6.943	70.0	-6.2	-20.9	56.9	51.3
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
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