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.

Dunes Near Ulyxis Rupes:   PSP_003347_1130   PSP_003624_1130   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-66.5

161.

4.22

-8.77

63.7

60.0

Light-Toned Layering in Ius Chasma:   PSP_003593_1725   ESP_058000_1725   (Interval in Earth days: 4239)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.48

275.

4.77

-11.1

51.7

34.5

Gullies in Newton Crater:   PSP_003675_1375   PSP_005877_1375   (Interval in Earth days: 172)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-42.2

201.

0

25.53

49.8

44.0

Fine Textures Near Headwaters of Warrego Valles:   PSP_003633_1385   PSP_004266_1385   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.1

267.

5.7

-9.82

49.8

42.3

Unnamed Fresh Crater Northeast of Ascraeus Mons:   PSP_003844_1995   PSP_004134_1995   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.23

260.

-0.4

26.39

63.0

60.2

Lobate Deposit and Mesa Near Reull Vallis:   PSP_003217_1355   ESP_046890_1355   (Interval in Earth days: 3403)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-44.3

105.

7.75

-8.47

56.9

61.5

Cover a Subset of Gullies Previously Identified in MOC Image M10-03905:   PSP_004196_1325   PSP_005251_1325   (Interval in Earth days: 82)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-47.2

19.4

-5.9

-28.1

44.3

43.4

Interesting Gullies:   PSP_004176_1405   PSP_005587_1405   (Interval in Earth days: 110)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.3

202.

8.88

-12.5

41.6

41.0

Layers and Fault in Crater in MOC Image R19-01820:   PSP_003168_1800   PSP_003880_1800   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.108

357.

-2.3

20.87

55.9

51.3

Small Meandering Channels:   PSP_003252_2195   PSP_003529_2195   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.88

219.

-0.5

-19.5

71.8

75.6


  


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