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.

Possible Collapse Feature in Impact Crater Ejecta:   PSP_005933_2200   ESP_011286_2200   (Interval in Earth days: 417)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.71

105.

-6.4

11.69

56.3

62.4

Scarp Likely Exposing Polar Layered Deposits in Area Not Well Observed:   PSP_005774_0915   ESP_023125_0915   (Interval in Earth days: 1352)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.2

212.

12.6

21.16

79.7

73.9

Aureum Chaos Mineralogical Variability:   PSP_006861_1765   ESP_094196_1765   (Interval in Earth days: 6805)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.34

332.

1.00

-15.8

40.0

36.6

Gullies:   PSP_006605_2120   PSP_007251_2120   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
31.46

118.

-3.9

11.81

43.9

40.1

Possible Exposure of Polar Layered Deposits in Area Not Well Observed:   PSP_004882_0880   PSP_004894_0920   (Interval in Earth days: 1)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.1

121.

11.7

11.47

68.6

67.9

Xanthe Terra Crater:   PSP_006598_1780   ESP_033326_1780   (Interval in Earth days: 2083)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.16

313.

2.29

24.68

37.1

37.0

Layered Deposit in Noachis Terra Crater:   PSP_005831_1300   PSP_006622_1300   (Interval in Earth days: 62)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-49.7

24.3

-21.

3.495

51.3

63.1

Large Region of Layering in Meridiani Planum:   PSP_006227_1810   ESP_011791_1810   (Interval in Earth days: 434)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.126

2.68

0

28.55

34.9

55.4

Layers Exposed in Central Peak-Pit of Unnamed Crater:   PSP_005201_1640   PSP_005913_1640   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.8

296.

5.02

22.96

33.2

32.4

Layers at the Head of Chasma Australe Exposed over 270 Degrees of Azimuth:   PSP_004788_0945   PSP_005079_0945   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-85.6

95.5

0

-16.3

65.3

69.7


  


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