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.

Fine Layers in Central Mound of Large Old Crater:   PSP_006187_1915   ESP_011395_1915   (Interval in Earth days: 406)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.35

13.5

0

17.38

37.1

56.5

Central Uplift in Runanga Crater:   PSP_006620_1530   PSP_010549_1530   (Interval in Earth days: 306)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.6

75.8

0.19

16.27

47.6

66.7

Northwest Hellas Region Landforms:   PSP_006845_1390   ESP_015943_1390   (Interval in Earth days: 709)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.5

54.2

2.86

28.43

60.2

63.1

Light-Toned Layering along Plains Southwest of Melas Chasma:   PSP_005584_1700   PSP_005729_1700   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.91

279.

4.99

21.16

32.8

31.4

Large Unnamed Fresh Crater West of Tomini Crater:   PSP_005748_1980   PSP_006671_1980   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.00

118.

4.14

-5.01

43.0

38.6

Mcmurdo Crater on the South Polar Layered Deposits:   PSP_004646_0955   PSP_004884_0955   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-84.4

1.54

0

-18.3

63.3

66.4

Gullies Cut into Light-Toned Rock:   PSP_006888_1410   ESP_016184_1410   (Interval in Earth days: 724)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.4

319.

2.83

-23.2

59.4

68.2

Seasonal Monitoring:   PSP_005750_0965   PSP_005921_0965   (Interval in Earth days: 13)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-83.6

99.6

-2.1

13.97

75.7

77.5

Polar Layered Deposit Stratigraphy Near Chasma Australe:   PSP_004722_0945   PSP_005052_0945   (Interval in Earth days: 26)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-85.3

94.8

0

-8.15

64.7

68.1

Central Peak with Layered Bedrock:   PSP_005683_1640   ESP_011458_1640   (Interval in Earth days: 450)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.7

96.8

5.59

18.89

32.6

57.3


  


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