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.

Gullied Slope:   ESP_067695_1430   ESP_068104_1430   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.7

222.

-7.1

23.60

48.2

52.8

Layered Terrain:   ESP_067570_1815   ESP_067702_1815   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.565

26.8

8.49

-8.15

39.7

41.0

Valleys in Crater South of Miyamoto Crater:   ESP_067347_1755   ESP_066529_1755   (Interval in Earth days: 64)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.36

353.

-10.

5.711

40.0

44.3

South Polar Residual Cap:   ESP_067625_0945   ESP_067665_0945   (Interval in Earth days: 3)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-85.5

5.73

4.61

-4.92

80.0

81.5

Collapse Pit in Graben with Ice Fill:   ESP_067627_2275   ESP_067970_2275   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
47.18

265.

5.14

23.64

64.0

58.4

Terrain Sample Northwest of Sytinskaya Crater:   ESP_067520_2235   ESP_068061_2235   (Interval in Earth days: 42)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.15

305.

4.04

14.32

62.6

55.5

Well-Preserved Impact Crater:   ESP_067461_2035   ESP_077458_2035   (Interval in Earth days: 778)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.43

118.

3.05

-10.3

50.3

42.0

Small Craters on South Polar Layered Deposits:   ESP_067412_0910   ESP_067176_0910   (Interval in Earth days: 19)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-89.0

56.8

27.7

22.52

77.5

74.5

Small Impact Crater Exposed by Erosion:   ESP_067455_1755   ESP_067930_1755   (Interval in Earth days: 37)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.48

286.

-3.2

8.213

39.3

40.2

Gullied Crater Walls:   ESP_067352_1360   ESP_067629_1360   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.9

222.

-8.8

14.12

47.3

49.8


  


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