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.

Possible Future Mars Landing Site of 2018 Joint Rover:   ESP_026270_1820   ESP_027747_1820   (Interval in Earth days: 115)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.165

350.

3.38

-8.58

50.3

53.3

Cratered Cones with Divergent Wakes Near Grjota Valles:   ESP_026369_1965   ESP_028413_1965   (Interval in Earth days: 159)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.52

167.

-8.3

7.177

44.8

50.8

Northern Plains Craters:   ESP_026446_2305   ESP_027158_2305   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.09

219.

0

16.82

42.3

43.0

Complex Superposition of Fractures:   ESP_026286_2235   ESP_026563_2235   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.31

269.

-3.0

-21.3

41.0

43.0

Fresh Crater:   ESP_026365_2260   ESP_027710_2260   (Interval in Earth days: 105)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
45.42

271.

1.37

20.86

41.0

45.7

Bedform Changes Southwest of Schiaparelli Crater:   ESP_026322_1720   ESP_027166_1720   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.72

13.0

-3.6

-18.2

56.9

59.2

Layers in Crater in Protonilus Mensae:   ESP_026518_2280   ESP_027863_2280   (Interval in Earth days: 105)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
47.87

53.4

5.71

26.90

41.3

47.3

Basin in Northeast Hellas Region:   ESP_026412_1525   ESP_026557_1525   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.2

78.2

0

15.95

70.4

69.9

Well-Exposed Bedrock Layers in Northern Hellas Planitia:   ESP_026492_1540   ESP_036052_1540   (Interval in Earth days: 745)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.9

54.4

-4.8

7.826

70.0

70.5

Meridiani Planum Terrain Sample:   ESP_026283_1810   ESP_026415_1810   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.156

354.

26.9

-16.8

49.2

52.9


  


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