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.

Flow Margin Fracturing Northwest of Elysium Mons :   ESP_048932_2135   ESP_049222_2135   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.05

139.

-2.6

22.16

64.2

59.3

Possible Flow Material at Bakhuysen Crater Rim :   ESP_048950_1575   ESP_049095_1575   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.4

14.6

0.32

15.89

32.0

29.9

Central Uplift of Crater in Tyrrhena Terra :   ESP_048921_1555   ESP_049066_1555   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.4

87.5

-9.7

5.579

32.9

30.8

Dipping Layers Near Reull Vallis :   ESP_048986_1415   ESP_058151_1415   (Interval in Earth days: 714)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.3

113.

3.21

20.49

33.8

33.2

Spider Topography :   ESP_048932_0970   ESP_040453_0970   (Interval in Earth days: 661)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-82.9

167.

5.54

20.66

62.6

65.3

Isolated Secondary Crater Cluster from Resen Crater in Hesperia Planum :   ESP_048973_1520   ESP_049540_1520   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.6

108.

-7.9

4.183

32.5

31.5

Crater with Steep Slopes :   ESP_048648_1365   ESP_048938_1365   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.3

344.

-10.

10.17

37.8

35.3

Tilted Block in Subsided Region South of Orson Welles Crater :   ESP_048873_1780   ESP_049651_1780   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.97

314.

2.45

12.36

39.7

31.5

Discontinuous Sinuous Ridge within Valley :   ESP_048681_1435   ESP_065903_1435   (Interval in Earth days: 1342)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.0

160.

6.13

20.21

34.3

43.0

Gullies and Arcuate Ridges in Nereidum Montes :   ESP_048623_1385   ESP_049124_1385   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.2

307.

-23.

-8.80

38.3

35.9


  


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