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.

Barchan to Linear to Transverse Dune Transition in Summer:   ESP_022775_1205   ESP_023065_1205   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-58.9

16.8

1.70

18.55

47.2

49.3

South Polar Layered Deposits:   ESP_023023_0925   ESP_023259_0925   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.5

150.

7.07

19.10

73.5

75.6

Fans in Non-Cryptic Ice-Free Terrain:   ESP_023013_0980   ESP_022987_0980   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-81.9

4.76

18.7

0.506

66.9

67.6

Sand Changes in Southern Hemisphere:   ESP_022776_1085   ESP_022644_1085   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-71.3

-0.4

-21.

-5.72

57.8

55.5

Interior Layered Deposits on Floor of Depression:   ESP_022706_1485   ESP_022772_1485   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.1

95.4

8.63

-13.5

32.6

34.2

Polar Layers Exposed on Promethei Lingula Surface:   ESP_022825_0970   ESP_023062_0970   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-82.7

113.

-4.0

11.10

66.6

68.8

Pitted Materials and Central Uplift of a 30-Kilometer Crater in Terra Sabaea:   ESP_022984_1605   ESP_023617_1605   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.1

63.9

7.46

-11.8

31.0

35.2

Layered Cliffs and Possible MSL Rover Landing Site in Libya Montes:   ESP_023049_1835   ESP_023471_1835   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.611

85.8

15.7

5.782

36.3

33.8

Bedrock Exposures in 20-Kilometer Diameter Crater in Kasei Valles:   ESP_022817_2110   ESP_023529_2110   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
30.80

297.

0.46

16.36

58.8

48.2

Anastomosing Slope Streaks:   ESP_022875_1900   ESP_022809_1900   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.01

157.

-11.

11.33

43.7

43.1


  


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