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.

Region Shows Differentially-Eroded Fan Deposits:   PSP_005829_1580   PSP_006686_1580   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.8

72.8

-8.0

3.642

35.7

45.6

Fresh High-Latitude Crater:   PSP_006924_2335   PSP_009864_2335   (Interval in Earth days: 230)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
53.11

44.5

-0.5

18.47

53.5

47.5

Large Shallow Crater on Edge of South Polar Layered Deposits:   PSP_005390_0935   PSP_005666_0935   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-86.5

232.

-1.3

14.58

72.8

75.6

Basal Exposure of South Polar Layered Deposits:   PSP_005049_1075   PSP_005247_1075   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-72.1

138.

1.11

-21.4

56.4

59.9

36 Gullies Previously Identified and Fully Described in MOC Image M03-03547:   PSP_005646_1360   ESP_022682_1360   (Interval in Earth days: 1327)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.7

34.1

-24.

-7.08

45.0

38.1

Mounds in Arcadia Region:   PSP_006852_2200   PSP_007142_2200   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.53

213.

-6.8

10.53

46.6

43.4

Potentially Very Recent Impact Markings:   PSP_005693_1650   ESP_011468_1650   (Interval in Earth days: 450)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.6

184.

1.26

15.00

32.9

57.3

Alluvial Fan in Crater East of Maja Valles:   PSP_006941_1825   PSP_007732_1825   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.684

308.

-8.3

7.693

39.9

45.8

Mound of Layers in East Candor Chasma:   PSP_006968_1735   PSP_007179_1735   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.28

290.

8.32

-4.23

41.6

45.0

Proposed MSL Site in Nili Fossae Trough:   PSP_005776_2010   ESP_012039_2010   (Interval in Earth days: 488)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.92

74.3

-6.8

-24.7

45.2

66.1


  


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