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.

Crater with Fractured Floor Deposit in Tartarus Colles :   ESP_057608_1950   ESP_058597_1950   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.87

169.

0

11.19

51.7

38.9

Terrain in Utopia Planitia :   ESP_057848_2110   ESP_058125_2110   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
30.58

96.4

13.5

3.206

60.2

57.0

Cross-Cut Alluvial Fans in Central Pit Crater Northwest of Hellas Planitia :   ESP_057890_1580   ESP_058167_1580   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.6

38.1

1.25

-18.6

31.1

31.6

Hummocky Texture on Ridge Associated with Hale Crater Ejecta :   ESP_057708_1425   ESP_057840_1425   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.2

326.

6.59

-17.9

33.4

34.9

Flow Feature Associated with Nearby Well-Preserved 6-Kilometer Crater :   ESP_057519_1545   ESP_057862_1545   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.1

84.0

-2.1

-13.2

34.2

32.3

Central Structure of Impact Crater :   ESP_057796_2075   ESP_067502_2075   (Interval in Earth days: 757)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.34

76.9

5.05

24.53

58.6

50.8

Tilted Layers in Electris Region :   ESP_057621_1430   ESP_058175_1430   (Interval in Earth days: 43)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.5

181.

3.44

-11.5

33.9

34.8

Test for Small Ancient Craters Near Nili Fossae :   ESP_057849_2030   ESP_058126_2030   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.85

72.2

-7.5

-18.5

55.1

52.1

South Polar Layered Deposits :   ESP_057770_0925   ESP_058006_0925   (Interval in Earth days: 19)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.6

125.

12.8

28.70

66.6

67.6

Possible Well-Exposed Ejecta Northeast of Holden Crater :   ESP_057576_1555   ESP_057721_1555   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.4

328.

-1.5

27.95

33.6

29.9


  


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