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.

Flow Deposits in Eastern Ladon Valles:   ESP_062099_1620   ESP_062534_1620   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-17.9

332.

-6.1

19.86

65.0

63.4

Clay-Bearing Landslide and Outcrop in Degraded Crater:   ESP_061990_1770   ESP_062056_1770   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.77

65.1

5.98

-13.8

54.3

55.8

Candidate Landing Site for 2020 and Sample Return Missions at Jezero Crater:   ESP_061950_1990   ESP_062095_1990   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.67

77.4

-27.

-11.1

46.6

45.5

Mesa in Chryse Planitia:   ESP_061954_1990   ESP_062020_1990   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.95

324.

8.90

-8.79

43.5

45.1

Ice-Filled Crater in North Polar Layered Deposits:   ESP_062085_2645   ESP_062203_2645   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.40

315.

0.89

14.85

59.7

59.7

Flow Margin in Phlegra Dorsa:   ESP_061854_2080   ESP_061920_2080   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.85

173.

8.37

-7.74

40.8

42.4

Dunes Dubbed La Jolla:   ESP_062168_2585   ESP_062115_2585   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
78.19

229.

-8.3

6.672

56.4

55.3

Crater Rim in Cydonia Mensae:   ESP_062098_2165   ESP_061742_2165   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.07

351.

10.5

-7.44

40.5

41.1

Ice-Filled North Polar Layered Deposit Crater:   ESP_062014_2645   ESP_062053_2645   (Interval in Earth days: 3)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.22

98.3

-2.3

11.61

59.6

59.2

Mound in Holden Crater:   ESP_061875_1545   ESP_062152_1545   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.2

326.

14.4

-8.23

68.6

70.2


  


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