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 Landing Site in Aram Chaos:   ESP_032178_1820   ESP_032468_1820   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.186

339.

-7.4

14.63

35.4

32.8

Light-Toned Materials Exposed along Ladon Valles Floor:   ESP_032218_1625   ESP_040539_1625   (Interval in Earth days: 649)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-17.4

328.

7.83

-3.22

32.1

34.1

South Polar Residual Cap in Summer:   ESP_032390_0925   ESP_032521_0925   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.3

5.67

8.59

19.38

81.5

82.7

Gullies with Light-Toned Apron Material Near Atlantis Chaos:   ESP_032408_1425   ESP_049168_1425   (Interval in Earth days: 1306)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.0

183.

-0.8

12.53

43.0

32.7

Dark Outcrops on South Polar Layered Deposits:   ESP_032202_0905   ESP_041078_0905   (Interval in Earth days: 692)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-89.3

94.5

28.3

24.91

78.6

80.0

Margin of Pedestal Crater in Malea Planum:   ESP_032440_1225   ESP_032572_1225   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-56.9

32.9

5.48

-22.0

57.2

61.0

Exposure of South Polar Layered Deposits:   ESP_032253_0920   ESP_040457_0920   (Interval in Earth days: 639)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.8

119.

24.1

8.824

78.4

70.9

Gullied Crater Walls:   ESP_032356_1465   ESP_023943_1465   (Interval in Earth days: 655)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.9

164.

-21.

-4.37

41.4

45.6

Lava Flow in Syria Planum:   ESP_032326_1605   ESP_032827_1605   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.1

259.

7.00

25.67

33.4

37.6

Dark V-Shaped Feature Cutting across Layers or Bands on a Slope:   ESP_032227_2040   ESP_040271_2040   (Interval in Earth days: 627)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.62

78.8

-8.7

3.583

46.4

56.7


  


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