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

Crater in Icaria Fossae Region with Intersecting Graben: ESP_011440_1335 ESP_011941_1335 (Interval in Earth days: 39)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-45.9	234.	-5.1	15.24	68.4	59.6
Shalbatana Vallis: PSP_010461_1845 ESP_016619_1845 (Interval in Earth days: 480)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
4.397	315.	0	0	54.7	45.8
Streamlined Landforms on Terraces of Ritchey Crater: PSP_010646_1510 ESP_016092_1510 (Interval in Earth days: 424)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-28.5	308.	7.57	-9.18	67.6	59.1
Central Uplift of a Large Impact Crater: PSP_010534_1620 ESP_051992_1620 (Interval in Earth days: 3230)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-17.8	125.	-4.5	-24.2	63.7	58.4
Cone at the Source of Athabasca Valles: PSP_010770_1905 ESP_011403_1905 (Interval in Earth days: 50)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
10.15	157.	16.7	-7.00	53.1	58.4
Central Peak of Gale Crater: PSP_010428_1745 ESP_016085_1745 (Interval in Earth days: 440)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-5.40	137.	4.52	-23.3	57.8	46.9
Possible MSL Landing Site in Gale Crater: ESP_011417_1755 ESP_011562_1755 (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
-4.44	137.	-15.	1.284	58.8	57.4
The North Pole of Mars: PSP_010545_2700 PSP_010586_2700 (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
89.98	-154	-25.	-25.6	76.8	77.4
Giza Region Stereo: ESP_011447_0950 ESP_011448_0950 (Interval in Earth days: 0)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-84.8	65.7	9.42	-17.5	86.7	89.1
Especially Bright Materials in Candor Chasma: ESP_011372_1730 ESP_012295_1730 (Interval in Earth days: 72)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-6.78	284.	5.39	20.7	57.4	53.0
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