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.

Surface Features Emanating from Alcove in Deuteronilus Mensae:   ESP_040787_2210   ESP_041222_2210   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.73

30.1

-6.7

26.93

63.2

55.1

Spider Terrain:   ESP_040789_0950   ESP_049334_0950   (Interval in Earth days: 666)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-85.0

13.6

3.96

-6.39

72.8

69.5

Patterned Ground on Braided Channel Near Steep Scarp:   ESP_041036_1460   ESP_040601_1460   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.7

80.7

3.24

-29.2

39.5

38.6

Light-Toned Layered Deposit within Hydrae Chasma:   ESP_040962_1735   ESP_049533_1735   (Interval in Earth days: 668)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.65

297.

-1.3

-12.3

34.1

32.5

Terracing Inside and Outside Degraded Crater Rim:   ESP_040785_2135   ESP_041286_2135   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.38

84.9

0.81

23.90

57.1

49.1

Exposure of South Polar Layered Deposits:   ESP_040914_0925   ESP_041124_0925   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.3

220.

8.72

22.05

76.7

79.0

South Polar Layered Deposits:   ESP_041021_0885   ESP_040835_0885   (Interval in Earth days: 14)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.7

291.

26.9

19.18

80.1

77.0

Fans and Polygons:   ESP_041061_0925   ESP_040849_0925   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.2

167.

8.68

21.52

79.1

74.5

Left Rim of Gullied Crater in Kaiser Crater:   ESP_040801_1335   ESP_047948_1335   (Interval in Earth days: 557)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.1

18.7

-0.0

-15.0

43.9

46.6

Low Albedo Wall Spurs in Coprates Chasma:   ESP_040949_1670   ESP_041305_1670   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.0

294.

-14.

4.235

34.6

34.7


  


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