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.

Interior Layered Deposits in Candor Chasma :   PSP_002696_1745   PSP_003197_1745   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.69

284.

0.15

26.47

55.7

52.3

Proposed MSL Site in NE Syrtis Major:   PSP_002809_1965   PSP_006000_1965   (Interval in Earth days: 248)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.45

76.5

0.07

23.03

58.5

38.5

Depositional Fan :   PSP_002387_1985   PSP_003798_1985   (Interval in Earth days: 110)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.48

77.4

1.71

-15.8

55.6

63.7

Southern Layered Mound and Floor in Gale Crater:   PSP_002464_1745   PSP_003176_1745   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.51

138.

2.93

21.29

55.7

52.8

Inverted Channels near Juventae Chasma:   PSP_003223_1755   PSP_003724_1755   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.31

296.

0

27.52

54.6

50.0

Edge along Gale Crater Interior Mound:   PSP_001488_1750   PSP_001752_1750   (Interval in Earth days: 20)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.83

137.

2.36

-16.1

56.5

57.7

Layers in a Central Mound in Gale Crater:   PSP_001422_1750   PSP_001620_1750   (Interval in Earth days: 15)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.98

137.

2.01

-12.5

56.7

57.6

Best Fan Surfaces in West Holden Crater:   PSP_001468_1535   PSP_002154_1530   (Interval in Earth days: 54)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.5

325.

6.55

-10.2

67.8

64.3

Nili Fossae Trough, Candidate MSL Landing Site:   PSP_003086_2015   PSP_003587_2015   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.12

74.2

-6.8

19.81

62.4

62.7

Proposed Strandline:   PSP_001820_1985   PSP_003442_1985   (Interval in Earth days: 126)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.25

77.3

1.02

-22.9

51.3

64.1


  


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