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.

Sinuous Ridge Emergent From Beneath Crater Ejecta:   ESP_072683_1825   ESP_072393_1825   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.445

148.

28.5

8.551

54.0

55.3

Chaos-Like Valley Southwest of Deuteronilus Mensae:   ESP_072622_2160   ESP_072833_2160   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.47

11.6

2.93

-6.19

57.0

60.5

Boundary Boulders:   ESP_071923_2260   ESP_071699_2260   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
45.42

13.8

20.3

-6.10

49.2

49.7

Varied Types of Rock in a Crater in Eos Chasma:   ESP_072413_1700   ESP_078980_1700   (Interval in Earth days: 512)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.78

324.

1.48

24.83

59.7

58.3

Candidate ExoMars Landing Site in Oxia Planum:   ESP_072307_1985   ESP_072241_1985   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.32

335.

-8.7

14.63

53.7

51.3

North Polar Layered Deposits Crater:   ESP_072095_2600   ESP_072003_2600   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.83

340.

8.87

-5.16

66.3

66.0

Modification of Ringed Crater:   ESP_072007_2485   ESP_072139_2485   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
68.45

234.

8.48

-8.32

59.3

62.3

Crater in Arabia Terra:   ESP_072398_2220   ESP_072464_2220   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.47

6.12

8.82

-8.40

55.0

57.3

Translucent Ice on Dunes South Site:   ESP_072321_2550   ESP_072268_2550   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
74.99

299.

-1.4

17.00

67.7

65.6

Dark Dune Field Topography in Bunge Crater:   ESP_072374_1460   ESP_072440_1460   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.4

311.

11.1

-11.4

70.3

71.2


  


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