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.

Inter-Plate Trough in Cerberus Palus:   ESP_032264_1840   ESP_057899_1840   (Interval in Earth days: 1997)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.021

150.

2.19

-7.32

34.9

41.3

Exposure of South Polar Layered Deposits:   ESP_032238_0920   ESP_032476_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

158.

27.6

21.28

77.9

82.4

Gullies with Bright Deposits in Dao Vallis:   ESP_032385_1455   ESP_024328_1455   (Interval in Earth days: 627)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.3

92.3

-10.

22.94

41.8

51.1

Terra Cimmeria Intra-Crater Barchan Dune Changes:   ESP_032475_1235   ESP_032607_1235   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-56.0

157.

1.83

-25.4

57.2

61.0

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

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

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

Knob on Polar Layered Deposits in Area Not Well Observed:   ESP_032178_0920   ESP_031992_0920   (Interval in Earth days: 14)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.1

55.4

11.4

21.44

78.8

74.6

Dunes:   ESP_032354_1165   ESP_023664_1165   (Interval in Earth days: 677)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-63.3

228.

-26.

-5.34

62.6

63.2

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


  


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