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.

Ismenius Cavus Channel:   ESP_089342_2145   ESP_090252_2145   (Interval in Earth days: 71)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.01

17.7

5.30

-17.5

47.4

58.3

Planned ExoMars Landing Ellipse Imaging in Oxia Planum:   ESP_089581_1995   ESP_089291_1995   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.24

335.

3.28

-24.9

50.3

51.5

Dune Interaction with Residual Polar Ice:   ESP_089286_2595   ESP_089405_2595   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.46

89.3

3.05

-13.8

61.3

63.6

Exposure of North Polar Layered Deposits:   ESP_089303_2605   ESP_089962_2605   (Interval in Earth days: 52)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.27

345.

0.31

14.90

62.1

69.6

Avalanche Scarp:   ESP_089280_2640   ESP_089386_2640   (Interval in Earth days: 8)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
83.76

236.

6.42

-8.01

63.6

65.4

Mamers Valles:   ESP_089329_2175   ESP_089606_2175   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.21

13.9

-10.

-29.1

48.8

52.9

Dune Interaction with Residual Polar Ice:   ESP_089589_2600   ESP_089470_2600   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.63

97.9

1.02

16.15

64.9

62.5

Characterize Possilbe Rotorcraft Landing Site:   ESP_089283_2205   ESP_089362_2205   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.97

189.

-7.1

19.14

48.3

46.5

Skylight Candidate near Elysium Mons:   ESP_089522_2090   ESP_089667_2090   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.91

145.

-3.6

11.04

49.5

49.3

Fan-Shaped Deposit in Arcadia Planitia:   ESP_089428_2200   ESP_089494_2200   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.86

188.

6.33

-9.62

48.3

50.2


  


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