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.

Polar Crater with Summer Ice and Central Uplift:   ESP_018479_2460   ESP_019323_2460   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
65.47

283.

3.50

-8.43

51.3

61.4

Seasonal Monitoring of Sublimation in Gypsum Source Region:   ESP_018335_2600   ESP_018309_2600   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.97

240.

8.59

-8.95

57.8

58.7

Rim and Ejecta of Very Fresh 7-Kilometer Diameter Impact Crater:   ESP_018268_2335   ESP_033854_2335   (Interval in Earth days: 1215)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
53.34

289.

-4.9

20.21

46.1

47.4

Layered Terrain in Aeolis Planum:   ESP_018181_1730   ESP_018893_1730   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.83

152.

-5.0

11.41

58.6

56.8

Relatively Young Crater Ejecta and Apron in Deuteronilus Mensae:   ESP_018423_2230   ESP_019056_2230   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.74

18.1

3.74

-12.5

44.0

50.4

North Polar Residual Cap:   ESP_018289_2655   ESP_018593_2655   (Interval in Earth days: 24)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
85.19

34.7

5.01

-9.35

61.3

63.9

Lava Channel and Cataract in South-Central Elysium Planitia:   ESP_018339_1820   ESP_018194_1820   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.117

157.

-0.8

-16.4

53.3

54.4

Dark Outcrop:   ESP_018292_1780   ESP_019492_1780   (Interval in Earth days: 94)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.92

0.09

11.0

-12.0

54.7

55.9

Cracks and Fans on Dunes:   ESP_018404_2610   ESP_018865_2610   (Interval in Earth days: 36)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.96

156.

6.25

24.73

59.0

62.0

North Polar Crater Change Detection:   ESP_018471_2645   ESP_018498_2645   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.32

120.

-0.4

-16.8

62.0

63.1


  


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