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.

Monitor Steep Slopes in Depression North of Ganges Chasma:   ESP_031032_1765   ESP_031177_1765   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.61

308.

-19.

-3.73

45.0

42.3

Reull Vallis Sample:   ESP_031092_1425   ESP_031237_1425   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.1

112.

5.11

19.31

36.1

34.2

Possible Pitted Impact Melt Pond on the Ejecta of Bakhuysen Crater:   ESP_031267_1565   ESP_031913_1565   (Interval in Earth days: 51)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.4

13.8

-6.3

22.74

34.8

30.6

Sediments in Valleys Upslope of Ladon Valles Basin:   ESP_030939_1600   ESP_031796_1600   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.9

327.

-2.4

17.48

38.4

30.6

Possible Fluvial Features in Golden Crater:   ESP_031005_1575   ESP_039405_1575   (Interval in Earth days: 654)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.0

326.

-5.8

8.33

37.4

43.5

Reull Vallis and Tongue-Shaped Landform in the Centauri Montes:   ESP_031119_1405   ESP_031264_1405   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.0

97.1

-11.

2.562

37.6

35.9

Light-Toned Materials Exposed within Holden Crater Secondary Crater:   ESP_031071_1605   ESP_030649_1605   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.4

325.

-19.

2.767

38.3

41.6

Flows Associated with Mojave Crater Secondaries:   ESP_031229_1895   ESP_040196_1895   (Interval in Earth days: 699)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.550

326.

1.62

22.38

48.5

46.8

Blocky Deposit on Floor of Melas Chasma:   ESP_030967_1715   ESP_031956_1715   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.64

282.

-8.4

-27.2

42.2

34.9

Possible Preserved Impact Melt Flow on the Ejecta of Bakhuysen Crater:   ESP_031201_1555   ESP_031056_1555   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.3

13.8

17.1

1.41

33.5

36.1


  


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