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.

Exposure of South Polar Layered Deposits:   ESP_085009_0905   ESP_085037_0905   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-89.5

289.

29.6

26.87

77.2

78.0

Possible Hydrothermal Setting in Northeast Syrtis Major Region:   ESP_085160_1970   ESP_085015_1970   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.88

76.6

-0.4

-17.1

43.5

46.0

Lighter-Toned Deposits in Young Crater:   ESP_085271_1870   ESP_085337_1870   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.156

287.

-1.6

-20.0

38.2

39.4

Sinuous Ridges on Both Sides of Scarp in Aeolis Planum:   ESP_084920_1730   ESP_085065_1730   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.73

151.

-1.5

13.33

35.5

34.1

Inverted Channels in Noachis Terra:   ESP_085294_1610   ESP_085637_1610   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.5

22.6

6.24

-17.7

36.3

41.6

South Polar Residual Cap:   ESP_084980_0915   ESP_067508_0915   (Interval in Earth days: 1361)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.3

340.

25.6

18.92

75.9

79.5

Phlegra Montes:   ESP_085038_2180   ESP_085117_2180   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.80

164.

-1.4

25.59

59.1

56.4

Tempe Fossae:   ESP_085099_2280   ESP_085231_2280   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
47.56

295.

15.0

-10.4

64.8

64.2

Layering Ridge near Surius Vallis:   ESP_085033_1255   ESP_085099_1255   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-54.2

312.

8.50

-5.42

51.4

53.2

Raised Glacier-Like Forms in Arabia Terra:   ESP_085043_2150   ESP_085109_2150   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.67

27.6

6.88

-10.0

56.2

56.3


  


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