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.

Lobate Feature on Slope on Northwest Hellas Region Rim:   ESP_023710_1425   ESP_024000_1425   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.0

46.4

-0.4

26.27

44.4

47.4

End of Trough in South Polar Residual Cap:   ESP_023504_0880   ESP_023703_0880   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.8

5.71

7.96

13.33

82.0

86.1

Possible Exposure of Polar Layered Deposits in Area Not Well Observed:   ESP_023715_0910   ESP_023756_0910   (Interval in Earth days: 3)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.8

316.

24.2

20.11

84.0

85.5

Gullies with Debris Aprons:   ESP_023810_1395   ESP_023955_1395   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.4

196.

0.83

14.61

48.1

49.7

Aeolis Planum:   ESP_023785_1745   ESP_067671_1745   (Interval in Earth days: 3420)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.55

154.

0

-21.5

32.9

41.2

Well-Preserved Gullied Crater:   ESP_023731_1405   ESP_024021_1405   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.9

195.

-25.

0.887

47.6

50.6

Proposed Landing Site in Jezero Crater:   ESP_023524_1985   ESP_023379_1985   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.33

77.5

-0.5

-11.8

41.0

43.2

Auqakuh Vallis Bedform Changes:   ESP_023696_2110   ESP_023762_2110   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
30.68

60.5

-7.2

-24.5

47.5

47.9

Eastern Wall of Chasma Australe along Margin of Promethei Lingula:   ESP_023590_0975   ESP_032530_0975   (Interval in Earth days: 697)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-82.4

101.

6.76

22.90

77.3

78.5

Possible Chloride Salts in Icaria Planum:   ESP_023716_1420   ESP_031918_1420   (Interval in Earth days: 639)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.5

242.

-1.3

-14.5

44.9

38.4


  


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