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.

Strange Dendritic Relief Features:   PSP_001950_2090   PSP_002240_2090   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.69

126.

-1.5

23.36

53.0

53.9

Light Mounds in Acidalia Region :   PSP_002457_2195   PSP_002536_2195   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.25

323.

2.18

27.51

61.6

60.5

Sharp-Looking Gullies :   PSP_002888_1400   PSP_004167_1400   (Interval in Earth days: 100)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.6

87.9

-8.1

14.24

61.4

41.4

Layering in Danielson Crater :   PSP_002944_1880   ESP_019835_1880   (Interval in Earth days: 1317)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.951

352.

-11.

10.60

58.1

52.8

Tributary of Shalbatana Vallis, As Seen in MOC Image R09-01983:   PSP_001930_1835   PSP_002431_1835   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.411

316.

-0.0

24.34

54.1

53.1

Incipient Gullies, As Seen in MOC Image M20-00901:   PSP_002146_1335   PSP_002423_1335   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.1

184.

6.03

-15.6

72.9

70.8

North Polar Layered Deposits Exposed Wall:   PSP_001488_2665   ESP_019158_2665   (Interval in Earth days: 1377)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
86.50

80.0

0.47

-8.93

70.0

70.7

Layered Deposit in an Arabia Region Crater :   PSP_002706_1870   PSP_003339_1870   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.783

10.2

-4.6

-19.3

56.6

59.0

Faulted Layers in Impact Crater in Meridiani Planum :   PSP_002733_1880   PSP_002878_1880   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.059

353.

-6.9

8.587

57.0

56.3

Wrinkle Ridge Cross-Cutting Relationships in Hesperia Planum :   PSP_002544_1540   PSP_002689_1540   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.8

116.

2.57

16.59

59.9

57.6


  


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