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.

Streamlined Form and Hill in Marte Vallis:   ESP_085156_1980   ESP_085433_1980   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.73

185.

7.29

-6.33

43.5

42.2

Hillslope Shapes on Holden Crater Rim:   ESP_085006_1550   ESP_085151_1550   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.7

325.

2.17

18.92

36.0

35.9

Landforms above Subsurface Radar Observations of South Polar Cap:   ESP_084946_1060   ESP_085078_1060   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-73.8

175.

-0.6

-14.4

65.2

68.1

Total Chaos:   ESP_083952_1925   ESP_084453_1925   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
12.25

303.

-0.2

-15.1

54.8

49.6

There’s No Place Like Terby!:   ESP_083921_1525   ESP_084422_1525   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.0

74.3

4.80

-10.2

38.7

36.4

Cross Cutting in a Crater:   ESP_085164_1620   ESP_085718_1620   (Interval in Earth days: 43)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-17.6

331.

7.82

-8.66

35.0

41.5

Terraced Impact Crater on Lobate Debris Apron:   ESP_084759_1385   ESP_084825_1385   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.9

232.

2.14

-19.6

40.6

42.6

Ridges on Crater Floor in Terra Sabaea:   ESP_084779_1510   ESP_085069_1510   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.6

44.1

6.57

26.75

35.6

36.0

Small Fresh Crater:   ESP_084536_1160   ESP_085195_1160   (Interval in Earth days: 51)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-63.8

208.

-2.9

29.34

52.6

59.7

Landforms above Subsurface Radar Observations of South Polar Cap:   ESP_084628_0935   ESP_084680_0935   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-86.3

250.

3.97

18.69

70.7

70.3


  


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