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.

Features in Nepenthes Mensae:   ESP_092305_1920   ESP_092384_1920   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.99

124.

-0.9

24.20

58.6

56.3

Landforms above Subsurface Radar Observations of South Polar Cap:   ESP_092633_0995   ESP_084840_0995   (Interval in Earth days: 607)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-80.2

200.

-21.

-7.26

61.7

69.1

Network of Channels on Rim of Newton Crater:   ESP_092632_1420   ESP_092698_1420   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.6

200.

-2.6

-25.5

40.1

41.4

Troughs overlying South Polar Layered Deposit:   ESP_092416_0905   ESP_083622_0905   (Interval in Earth days: 685)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-89.3

8.90

28.4

26.90

64.8

64.9

Holden Crater Sedimentary Fan:   ESP_092456_1525   ESP_092667_1525   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.9

325.

0.76

-25.0

41.6

41.2

Crater-Related Pitted Materials in 3-Kilometer Crater in Nepenthes Planitia:   ESP_092411_1960   ESP_092622_1960   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.73

108.

5.50

-22.3

59.7

59.6

Triangular Scars on Hillslopes:   ESP_092549_1335   ESP_092325_1335   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.2

308.

3.67

-16.2

42.4

46.3

Alluvial Fan in Kasei Vallis:   ESP_092602_2030   ESP_092681_2030   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.70

292.

-2.3

24.40

63.3

61.0

Landforms above Subsurface Radar Observations of South Polar Cap:   ESP_092561_0990   ESP_084729_0990   (Interval in Earth days: 610)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-81.0

352.

10.6

-5.34

60.0

68.1

South Polar Glacier Crevasses:   ESP_092682_0915   ESP_092589_0915   (Interval in Earth days: 8)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.6

323.

22.6

26.11

64.9

64.3


  


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