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.

Fresh Irregular Crater in Tyrrhena Terra :   PSP_010113_1575   ESP_062503_1575   (Interval in Earth days: 4082)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.0

100.

-3.9

8.055

67.6

67.0

Possible Flute Casts in Ares Vallis:   PSP_009722_1960   PSP_009867_1960   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.92

329.

2.51

17.22

48.9

48.1

Polar Layered Deposits Unconformity:   PSP_010048_2615   PSP_010509_2615   (Interval in Earth days: 36)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
81.49

49.1

-3.5

16.55

63.8

68.5

High-Latitude Exposure of North Polar Layered Deposits:   PSP_010100_2675   PSP_010457_2675   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.29

32.0

-5.8

-15.5

68.3

73.1

Small Shield Covering the Noctis Fossae:   PSP_010305_1780   PSP_010661_1780   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.91

256.

-7.0

-0.74

57.3

56.9

Unconformities in North Polar Layered Deposits:   PSP_010124_2650   PSP_010242_2650   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.81

128.

-7.7

7.364

67.0

67.7

Clay-Bearing Unit in the Western Arabia Region:   PSP_009735_1985   PSP_009880_1985   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.19

335.

-7.7

7.217

49.1

48.4

Fresh 8-Kilometer Diameter Impact Crater:   PSP_009625_1900   ESP_016060_1900   (Interval in Earth days: 501)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.793

98.5

4.97

-22.4

50.7

41.9

High-Latitude Exposure of North Polar Layered Deposits:   PSP_009301_2720   PSP_009528_2680   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
88.07

204.

-7.9

-21.1

63.9

64.7

Light-Toned Deposits and Possible Fluvial Channels on Floor of Ius Chasma:   PSP_010146_1720   PSP_010568_1720   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.96

277.

-4.7

-18.8

59.9

60.5


  


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