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.

Well-Preserved Impact Crater:   ESP_015905_2235   ESP_016182_2235   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.91

3.36

3.72

-15.9

45.9

45.8

Athabasca Valles:   ESP_016071_1890   ESP_024708_1890   (Interval in Earth days: 673)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.934

155.

7.83

-16.8

39.6

38.8

Stranded Lobe of Material with Associated Ridge on Valley Floor:   ESP_016238_2180   ESP_017161_2180   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.54

273.

-3.4

6.789

42.5

40.5

Gullied Crater Wall:   ESP_015950_1395   ESP_016451_1395   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.3

225.

4.65

25.21

64.5

70.3

Sinuous Ridge at Contact Between Lineated Valley Fill and Plains Material:   ESP_016142_2240   ESP_080745_2240   (Interval in Earth days: 5033)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.67

13.6

-3.2

20.12

45.2

49.8

Cerberus Fossae Cutting Hill:   ESP_016229_1895   ESP_016862_1895   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.130

162.

4.10

-9.74

40.9

46.1

Mounds on Hrad Vallis Mudflow:   ESP_016256_2155   ESP_016322_2155   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.06

142.

-2.8

-19.2

41.7

43.0

Juventae Region Mound and Possible Sulfate-Rich Terrain:   ESP_015934_1760   ESP_016646_1760   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.74

298.

0

21.43

42.9

48.4

Noachis Terra Sample:   ESP_016182_1560   ESP_016815_1560   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.5

9.41

6.53

-7.78

56.2

64.3

Central Peak of 70-Kilometer Diameter Impact Crater in Terra Sabaea:   ESP_016114_1580   ESP_016470_1580   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.9

66.7

-6.2

4.62

55.0

58.8


  


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