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.

South Polar Residual Cap in Late Summer:   ESP_032565_0910   ESP_032538_0910   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.9

280.

23.2

25.63

84.9

84.2

Migrating and Static Sand Ripples on Mars:   ESP_032616_1275   ESP_032748_1275   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-52.2

267.

3.02

-26.0

56.8

60.7

Lava against an Impact Crater in Elysium Planitia:   ESP_018537_1860   ESP_019170_1860   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.980

150.

5.55

-19.2

51.1

53.8

Possible Cyclic Bedding within a Crater in Arabia Terra:   ESP_018714_1890   ESP_019347_1890   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.969

358.

6.46

-18.9

50.0

53.4

Pitted Terrain Associated with Lava Flow:   ESP_032395_2070   ESP_032672_2070   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
26.74

170.

-0.5

-26.7

46.1

45.3

Exposure of South Polar Layered Deposits:   ESP_032401_0920   ESP_032650_0920   (Interval in Earth days: 19)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.9

93.8

8.93

20.48

82.8

85.6

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

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

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

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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