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.

Inverted Channel in Arabia Terra:   ESP_070526_1915   ESP_070737_1915   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.32

4.50

-7.8

-20.1

53.9

54.8

Crater in Arabia Terra:   ESP_070460_2210   ESP_071093_2210   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.77

2.16

-0.6

-25.4

46.6

48.9

Terraced Crater:   ESP_070454_2235   ESP_071456_2235   (Interval in Earth days: 78)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.08

164.

6.87

23.14

46.0

45.5

Circular Depression and Outlet in Hebrus Valles:   ESP_070772_1995   ESP_071062_1995   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.43

127.

-16.

6.172

51.3

49.3

Possible Phyllosilicate-Rich Outcrop in Walls South of Aurorae Chaos:   ESP_070066_1680   ESP_069565_1680   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.8

325.

17.4

-6.56

63.6

62.4

Dipping Layers Against Mounds in Northern Mid-Latitudes:   ESP_070036_2195   ESP_070458_2195   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.31

58.8

4.74

-16.8

46.9

48.0

Features in Hebrus Valles:   ESP_070205_1995   ESP_070495_1995   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.37

127.

-1.6

17.04

50.4

48.7

Small Lobe of Glacial Cover on Fresh Impact Crater:   ESP_070120_2195   ESP_070331_2195   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.16

285.

4.59

-6.81

46.7

47.3

Alluvial Fans in Ganges Chasma:   ESP_070185_1715   ESP_071899_1715   (Interval in Earth days: 133)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.34

317.

-6.0

19.25

63.5

58.8

Layering in Western Arabia Terra:   ESP_070065_1900   ESP_070355_1900   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.829

351.

-4.9

14.56

54.1

52.8


  


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