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.

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

Well-Preserved Gullied 15-Kilometer Impact Crater:   ESP_040964_1305   ESP_057856_1305   (Interval in Earth days: 1316)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-49.1

249.

-4.2

5.903

48.2

38.7

Pits on South Polar Layered Deposits:   ESP_040888_0930   ESP_041151_0930   (Interval in Earth days: 20)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.1

234.

-0.7

5.799

77.4

80.7

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

South Polar Layered Deposits:   ESP_041015_0910   ESP_040779_0910   (Interval in Earth days: 19)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.8

328.

25.9

21.66

78.3

75.2

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

Collapse Pit on South Polar Layered Deposits:   ESP_040913_0920   ESP_040846_0920   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.9

246.

14.8

26.48

76.7

74.6


  


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