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 Debris Aprons in Tyrrhena Terra:   ESP_031805_1545   ESP_031950_1545   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.2

84.1

3.68

21.79

32.2

31.3

Valleys in Tyrrhena Terra:   ESP_031817_1410   ESP_031751_1410   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.8

118.

5.17

22.85

36.9

35.1

Eastern Valles Marineris Bedrock Stratigraphy and Falling Dunes:   PSP_010277_1650   PSP_010699_1650   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.6

302.

-8.0

-24.2

63.3

63.2

Sedimentary Bedrock Diversity in Terby Crater:   ESP_031212_1525   ESP_031278_1525   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.1

73.9

17.1

-4.75

33.2

34.5

South Polar Layered Deposit Spiral Troughs during Katabatic Wind Season:   ESP_031048_0945   ESP_031100_0945   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-85.4

289.

-13.

2.826

65.5

64.1

Well-Preserved Crater in Hesperia Planum:   ESP_031171_1610   ESP_032160_1610   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.8

113.

1.89

-8.45

35.8

33.3

USGS Dune Database 2280-788 Changes:   ESP_031194_1010   ESP_031141_1010   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-78.7

228.

-14.

3.468

60.1

58.8

Monitor Steep Slopes in Depression North of Ganges Chasma:   ESP_031032_1765   ESP_031177_1765   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.61

308.

-19.

-3.73

45.0

42.3

Sediments in Valleys Upslope of Ladon Valles Basin:   ESP_030939_1600   ESP_031796_1600   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.9

327.

-2.4

17.48

38.4

30.6

Reull Vallis Sample:   ESP_031092_1425   ESP_031237_1425   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.1

112.

5.11

19.31

36.1

34.2


  


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