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.

Many Small Cones in Amazonis Planitia:   ESP_021990_1985   ESP_022412_1990   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.78

198.

-4.5

-18.4

59.5

56.0

Well-Preserved 5-Kilometer Diameter Impact Crater:   ESP_021767_1315   ESP_022400_1315   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-48.2

173.

6.74

-8.25

43.6

40.1

Well-Preserved Flow-Ejecta Crater East of Juventae Chasma:   ESP_021683_1735   ESP_057933_1740   (Interval in Earth days: 2824)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.25

301.

5.27

14.08

47.4

34.0

Hematite in Eos Chasma:   ESP_021775_1665   ESP_022408_1665   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.3

311.

-3.6

-23.2

44.4

38.4

Central Uplift with Layers and Clays:   ESP_021688_1325   ESP_021754_1325   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-47.2

170.

2.61

-14.9

44.6

45.1

Mounds North of Simud Valles Region Chaos:   ESP_021880_1950   ESP_030359_1950   (Interval in Earth days: 661)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.75

320.

4.40

-21.0

57.2

60.9

Northern Part of Asimov Crater Ring Trough:   ESP_021694_1330   ESP_021760_1330   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.4

4.90

21.1

4.178

42.9

43.4

Mesas and Buttes of Hydraotes Chaos:   ESP_021893_1805   ESP_031163_1805   (Interval in Earth days: 722)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.634

327.

3.40

22.57

48.7

42.4

Bedform Changes in Aureum Chaos:   ESP_021906_1765   ESP_022183_1765   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.64

333.

-1.9

-28.1

46.7

45.5

Fractures and Uplifted Portion of Floor of Echus Chasma:   ESP_021908_1810   ESP_021842_1810   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.856

279.

-17.

4.9

50.1

49.2


  


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