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.

Recent Crater in Southern Mid-Latitudes:   ESP_066067_1350   ESP_066476_1350   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-44.6

8.27

-1.5

-22.4

44.2

43.5

Valley Cutting Ejecta of Crater and Associated Sinuous Ridge:   ESP_065902_1685   ESP_065968_1685   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.3

185.

7.46

-6.99

47.9

48.2

Raided Curvilinear Ridges:   ESP_066022_1755   ESP_065956_1755   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.63

151.

-7.5

6.58

50.4

50.1

Bisected Polygonal Bedrock:   ESP_065918_1935   ESP_083234_1935   (Interval in Earth days: 1349)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
13.13

106.

-3.5

4.659

60.4

61.0

Lobate Flows in Phlegra Dorsa:   ESP_065810_2130   ESP_075016_2130   (Interval in Earth days: 717)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.59

171.

-2.4

6.659

73.2

69.7

Mounds in Oxia Colles:   ESP_065857_1990   ESP_065725_1990   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.87

331.

-12.

14.58

64.9

63.7

Elongated Collapse Pit in Ceraunius Fossae:   ESP_066005_2110   ESP_074143_2110   (Interval in Earth days: 634)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
30.54

250.

-3.7

-15.7

71.0

72.0

Layered Bedrock:   ESP_065747_1740   ESP_065958_1740   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.04

95.2

6.12

24.74

51.5

48.1

Candidate Recent Impact Site:   ESP_065754_1820   ESP_073681_1820   (Interval in Earth days: 617)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.910

264.

-5.6

4.297

55.7

57.6

Leveed Candidate Mudflow:   ESP_065910_1995   ESP_066042_1995   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.36

323.

1.75

-22.4

63.9

64.6


  


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