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.

Gullies in Southern Latitude Crater:   PSP_005701_1445   PSP_005991_1445   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.2

328.

0.44

26.02

39.3

41.2

Ringed Pit in Tractus Fossae:   PSP_005677_2055   ESP_011597_2055   (Interval in Earth days: 462)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.97

256.

-3.0

22.36

49.0

60.5

Light-Toned Outcrops in Noctis Labyrinthus:   PSP_006692_1740   ESP_024427_1740   (Interval in Earth days: 1382)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.99

267.

1.10

14.97

39.0

37.4

Graben in Eastern Olympus Mons:   PSP_005678_1995   PSP_005744_1995   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.44

230.

-7.4

-26.8

45.5

46.1

Small Fresh Crater:   PSP_005567_1690   ESP_023948_1690   (Interval in Earth days: 1432)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.6

24.5

-11.

8.2

33.9

34.3

Diverse Stratigraphic Layers Exposed in Depression:   PSP_006290_1590   PSP_010575_1590   (Interval in Earth days: 334)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.8

85.3

0

16.21

39.8

63.6

Central Uplift in Runanga Crater:   PSP_006620_1530   PSP_010549_1530   (Interval in Earth days: 306)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.6

75.8

0.19

16.27

47.6

66.7

Large Unnamed Fresh Crater West of Tomini Crater:   PSP_005748_1980   PSP_006671_1980   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.00

118.

4.14

-5.01

43.2

38.6

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

56.5

60.0

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

45.2

38.1


  


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