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.

Stratigraphy of Rocks in Claritas Fossae Region:   ESP_012995_1530   ESP_030902_1530   (Interval in Earth days: 1395)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.9

258.

-7.1

4.769

43.5

37.3

Bright Gully Deposits in Western Hale Crater:   ESP_013230_1445   ESP_014074_1445   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.0

322.

8.51

-20.1

39.3

37.8

Possible Fan Delta:   ESP_013531_2140   ESP_022036_2140   (Interval in Earth days: 663)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.87

17.5

-8.5

21.35

68.7

68.8

Light-Toned Outcrop in Hummock of Iani Chaos:   ESP_013717_1790   ESP_013862_1790   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.05

342.

5.13

18.19

42.1

39.5

Wrinkle Ridge in Lunae Palus:   ESP_014022_1950   ESP_014167_1950   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.94

294.

-7.9

7.828

48.7

45.9

Light-Toned Outcrops Near Crater Rim in Arabia Terra:   ESP_014165_1985   ESP_022314_1985   (Interval in Earth days: 635)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.07

349.

2.28

28.31

48.4

53.8

Well-Preserved 3 Kilometer Diameter Impact Crater:   ESP_012991_1335   ESP_013624_1335   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-45.9

9.53

3.76

-12.3

44.3

40.8

Exposure of Layered Sequence in Terby Crater:   ESP_013160_1530   ESP_074031_1530   (Interval in Earth days: 4743)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.9

74.0

-8.4

2.702

41.5

52.0

North Wall of Ritchey Crater:   ESP_013125_1520   ESP_013758_1520   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.9

309.

0.17

-22.9

41.2

37.0

Central Structure of a Large Impact Crater:   ESP_013134_1610   ESP_021494_1610   (Interval in Earth days: 652)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.6

62.6

-6.3

14.94

43.1

44.9


  


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