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.

Baldet Crater Dune Changes:   ESP_080229_2030   ESP_080295_2030   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.68

65.8

1.70

-15.0

48.5

50.2

Light-Toned Exposures near Voeykov Crater:   ESP_080340_1465   ESP_080274_1465   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.0

283.

-1.3

15.81

77.0

76.2

High-Latitude Exposure of North Polar Layered Deposits:   ESP_080218_2680   ESP_079956_2680   (Interval in Earth days: 20)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.72

307.

-7.8

-23.6

65.0

64.2

Frost-Free Dunes in Viking 2 Image 544B05:   ESP_080437_2570   ESP_080490_2570   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
76.66

130.

7.66

-7.69

59.3

61.0

A Fissure Vent East of Olympus Mons:   ESP_080579_1955   ESP_080790_1955   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.48

232.

5.92

-6.42

51.4

53.1

Eroded Sedimentary Rock Layers:   ESP_080568_1670   ESP_080779_1670   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.7

176.

-1.1

-14.0

63.8

64.2

Crustal Blocks in the Walls of Coprates Chasma:   ESP_080616_1640   ESP_078282_1640   (Interval in Earth days: 181)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.6

304.

22.8

-1.64

63.6

58.0

Preserved Meanders in Jezero Crater Outlet:   ESP_079846_1990   ESP_079701_1990   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.72

78.4

29.1

12.20

46.0

47.2

Small Delta or Fan:   ESP_080135_1830   ESP_080280_1830   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.140

114.

-7.4

16.94

56.2

54.6

Dune Interaction with Residual Polar Ice:   ESP_080121_2605   ESP_079673_2605   (Interval in Earth days: 35)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.53

98.1

23.9

9.047

58.0

57.0


  


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