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_004145_1455   ESP_013098_1455   (Interval in Earth days: 698)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.3

329.

-0.1

-21.4

42.1

43.2

Fresh Small Crater in Daedalia Planum:   PSP_003990_1455   ESP_047597_1455   (Interval in Earth days: 3398)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.3

240.

7.67

-10.3

43.6

48.6

Gullies in the North-Facing Wall of a Crater:   PSP_003215_1405   PSP_003492_1405   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.9

160.

-6.5

-26.6

56.4

54.0

Light-Toned Outcrops in the Plains Between Melas and Candor Chasma:   PSP_004318_1730   PSP_004740_1730   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.84

282.

-3.1

-15.3

45.8

41.7

Mangala Valles Cataract:   PSP_003991_1645   PSP_004347_1645   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.3

210.

0

10.73

46.2

41.2

Unnamed Well-Preserved Crater within the Isidis Basin:   PSP_003560_1900   PSP_005828_1900   (Interval in Earth days: 177)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.16

94.5

0.61

10.89

58.6

37.6

Gullies in Crater in South Aonia Terra :   PSP_003698_1295   ESP_014009_1295   (Interval in Earth days: 804)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-50.0

294.

5.99

23.69

51.1

41.4

Low Shield with Radial Flows East of the Olympica Fossae:   PSP_003818_2040   PSP_004108_2040   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.71

249.

-3.0

23.54

65.9

63.5

Subset of Gullies Previously Identified in Dunes in MOC Image M19-01170:   PSP_003682_1250   PSP_003748_1250   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-54.5

12.8

0.14

-13.7

53.3

53.3

Light-Toned Layering in Labyrinthus Noctis Pit:   PSP_003910_1685   PSP_005400_1685   (Interval in Earth days: 116)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.1

261.

0

14.87

48.2

32.3


  


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