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.

Hadriacus Mons Southwestern Caldera Wall:   ESP_077446_1490   ESP_085674_1490   (Interval in Earth days: 642)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-30.6

92.4

-8.3

6.14

56.7

46.3

Chaos Region in Ariadnes Colles:   ESP_077232_1445   ESP_077509_1445   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.2

172.

-5.3

7.105

55.9

59.7

Streamlined Landforms Adjacent to Shalbatana Vallis:   ESP_077332_1895   ESP_078255_1895   (Interval in Earth days: 71)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.454

317.

-4.1

4.45

39.7

45.0

Origin of Channels in Southern Low-Latitudes:   ESP_077368_1685   ESP_078080_1685   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.2

58.0

-5.7

10.09

44.8

52.5

Mounds in Oxia Colles:   ESP_077173_2055   ESP_080918_2055   (Interval in Earth days: 292)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.45

334.

2.01

13.86

42.2

50.9

Hydrated Materials in Columbus Crater:   ESP_077218_1505   ESP_077640_1505   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.2

193.

0

23.47

51.7

56.7

Southern Canyon Wall in East Coprates Chasma:   ESP_077227_1645   ESP_076739_1645   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.4

305.

1.47

-23.9

44.3

40.4

Channel in Terra Cimmeria:   ESP_077481_1415   ESP_086355_1415   (Interval in Earth days: 692)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.4

217.

6.91

28.75

61.4

60.7

Recent Crater:   ESP_077370_2130   ESP_077858_2130   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.80

357.

-2.7

-25.4

44.7

45.2

Alluvial Fan in Kasei Valles:   ESP_077148_2035   ESP_084809_2035   (Interval in Earth days: 597)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.42

296.

0.66

22.69

41.6

50.3


  


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