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.

Well-Preserved 4-Kilometer Impact Crater:   ESP_083095_1535   ESP_083240_1535   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.2

307.

-5.3

9.499

49.9

46.9

Fresh Crater near Ice-Rich Terrain:   ESP_083188_1295   ESP_083254_1295   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-50.3

290.

7.09

-8.45

50.5

50.7

Channel Edge with Overbank Flow Deposits:   ESP_083033_1835   ESP_082967_1835   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.456

195.

7.43

29.20

57.0

55.5

Eroded Landform in Chryse Planitia:   ESP_083121_1940   ESP_083767_1940   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
13.87

312.

-4.9

22.98

62.5

56.4

Flow Features on Ice-Rich Plateau on Malea Patera:   ESP_083276_1165   ESP_083144_1165   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-63.1

53.5

-7.0

15.29

55.0

55.2

Channel Entering Crater:   ESP_082956_1395   ESP_083378_1395   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.3

143.

4.73

-7.28

51.9

46.6

Pitted Material:   ESP_083282_1425   ESP_083928_1425   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.2

242.

4.8

21.65

46.8

37.9

Ariadnes Colles:   ESP_083100_1450   ESP_083588_1450   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.6

171.

3.68

-22.4

49.2

44.5

Planned ExoMars Landing Site in Oxia Planum:   ESP_083041_1980   ESP_082975_1980   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.80

335.

2.09

23.42

64.3

62.7

Channel in Valley near Tyrrhena Patera:   ESP_083076_1590   ESP_083142_1590   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.6

104.

3.93

-19.6

50.0

51.0


  


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