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.

Small Delta or Fan:   ESP_075615_2120   ESP_084239_2120   (Interval in Earth days: 672)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
31.94

20.6

4.68

21.07

62.7

64.3

Knobs in Chryse Planitia:   ESP_075604_1990   ESP_076593_1990   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.85

322.

3.53

15.48

53.2

41.4

Channel Head in Newton Crater:   ESP_075767_1405   ESP_076545_1405   (Interval in Earth days: 60)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.3

200.

-6.7

10.34

39.2

46.5

Veins in Ariadnes Colles Deposits:   ESP_075623_1450   ESP_082678_1450   (Interval in Earth days: 550)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.6

171.

-4.3

29.02

37.0

53.1

Channel Entering Orson Welles Crater:   ESP_075789_1785   ESP_076000_1785   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.52

313.

8.57

-2.18

38.6

37.7

Extra-Crater Sinuous Ridge:   ESP_075559_1185   ESP_075414_1185   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-61.3

121.

7.74

-6.12

49.0

49.0

Channel West of Eberswalde Crater:   ESP_075670_1555   ESP_075525_1555   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.1

325.

12.5

-9.22

34.1

36.3

Lobate Debris Apron on Floor of Barnard Crater:   ESP_075825_1190   ESP_076537_1190   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-60.7

60.4

2.28

24.69

51.3

60.5

Site Dubbed the Forks:   ESP_075511_0950   ESP_075195_0950   (Interval in Earth days: 25)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-85.0

13.7

8.41

-5.71

65.6

64.6

Crater with Steep Slopes:   ESP_075560_1880   ESP_093783_1880   (Interval in Earth days: 1420)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.924

85.0

3.56

18.20

46.5

38.8


  


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