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.

Sediment Lens in Jezero Crater Outlet :   ESP_048631_1990   ESP_049343_1990   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.68

78.6

4.85

19.37

55.8

46.5

Fractured Terrain North of Oudemans Crater :   ESP_048756_1735   ESP_048822_1735   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.26

268.

8.63

-16.0

38.4

39.3

Possible Flow Material at Bakhuysen Crater Rim :   ESP_048950_1575   ESP_049095_1575   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.4

14.6

0.32

15.89

32.0

29.9

Branched Trough and Pit Feature Associated with Curvilinear Ridge :   ESP_048990_1845   ESP_049346_1845   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.499

358.

4.92

17.76

42.0

37.0

Western Ejecta and Rays of Istok Crater :   ESP_048901_1345   ESP_047754_1345   (Interval in Earth days: 89)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-45.1

273.

16.9

0

35.7

48.1

Central Uplift of Crater in Tyrrhena Terra :   ESP_048921_1555   ESP_049066_1555   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.4

87.5

-9.7

5.579

32.9

30.8

Isolated Secondary Crater Cluster from Resen Crater in Hesperia Planum :   ESP_048973_1520   ESP_049540_1520   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.6

108.

-7.9

4.183

32.5

31.5

Polar Pit Gullies :   ESP_048819_1115   ESP_048687_1115   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-68.5

1.53

-5.7

13.54

51.4

50.0

Folded Layers on Floor of Ius Chasma :   ESP_048993_1725   ESP_049138_1725   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.56

279.

-8.7

8.232

36.3

33.7

Nili Patera :   ESP_048671_1890   ESP_092162_1890   (Interval in Earth days: 3389)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.711

67.5

8.01

22.9

48.2

56.1


  


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