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.

High-Latitude Exposure of North Polar Layered Deposits:   PSP_010808_2720   ESP_028150_2680   (Interval in Earth days: 1351)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.93

95.5

-6.3

-11.4

79.4

74.3

Well-Preserved Impact Crater on Northern Plains:   PSP_010559_2170   ESP_016005_2170   (Interval in Earth days: 424)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.54

155.

5.58

-8.20

52.5

43.4

Complex Morphology in Acidalia Region:   ESP_011384_2185   ESP_011661_2185   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.01

310.

7.35

-13.2

63.5

68.9

Mesas with Circumferential Depressions Near Kasei Valles:   ESP_011319_2100   ESP_011464_2100   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
29.64

289.

-20.

-7.41

62.3

62.9

Section of Wall Rock on the South Rim of Coprates Chasma:   PSP_010501_1645   ESP_016026_1645   (Interval in Earth days: 431)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.4

305.

5.32

23.12

62.0

48.0

Central Uplift of an Impact Crater:   PSP_010745_1465   ESP_028006_1465   (Interval in Earth days: 1345)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.2

126.

5.23

-17.2

69.4

71.8

Light-Toned Layering South of Ius Chasma with Unusual Morphology:   PSP_010423_1720   ESP_016726_1720   (Interval in Earth days: 491)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.01

275.

-10.

7.863

60.0

52.5

Possible MSL Landing Site in Holden Crater:   ESP_011397_1535   ESP_011898_1535   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.3

324.

3.35

27.36

61.3

54.6

Flow Feature in Southern Utopia Planitia:   ESP_011497_1965   ESP_064454_1965   (Interval in Earth days: 4126)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.22

110.

-4.3

-24.5

59.6

61.7

Crater Wall in Chryse Planitia:   PSP_010408_2070   ESP_045906_2070   (Interval in Earth days: 2766)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
26.88

319.

2.47

-6.79

50.6

48.1


  


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