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.

Kasei Valles Alluvial Fans and Flood Terrace:   ESP_089820_2025   ESP_089675_2025   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.03

290.

-0.2

-16.9

51.7

52.1

Survey of Terrain around Ice-Exposing Crater:   ESP_089639_2195   ESP_089507_2195   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.10

190.

-9.9

20.77

51.6

47.5

Sample of Scalloped Terrain West of Erebus Montes:   ESP_089349_2195   ESP_089072_2195   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.37

187.

-8.3

14.20

48.9

44.9

Dune Interaction with Residual Polar Ice:   ESP_089273_2595   ESP_089365_2595   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.28

88.0

-3.9

11.81

61.5

61.4

Thermal Anomaly in Young Lava Flows of Elysium Region:   ESP_089284_1970   ESP_089429_1970   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.03

163.

2.69

16.88

49.6

48.9

Layering in Southern Lucus Planum:   ESP_089336_1720   ESP_089481_1720   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.84

187.

4.06

19.82

59.8

58.4

Light-Toned Mesas in Arcadia Planitia:   ESP_089560_2260   ESP_089336_2260   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
45.44

183.

12.9

-21.3

49.9

50.8

Dune Interaction with Residual Polar Ice:   ESP_089589_2600   ESP_089470_2600   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.63

97.9

1.02

16.15

64.9

62.5

Features around Crater in Terra Sabaea:   ESP_089319_2205   ESP_089385_2205   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.93

284.

8.56

-7.88

47.1

49.1

Layering in Lucus Planum:   ESP_089244_1710   ESP_089521_1710   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.00

178.

8.29

-21.2

60.3

61.9


  


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