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.

Light-Toned Fan-Like Features in Crater in Chryse Chaos:   ESP_013256_1885   ESP_022104_1885   (Interval in Earth days: 689)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.534

327.

-1.4

-13.8

53.6

52.2

Strike Slip Fault in Amazonis Planitia:   ESP_012799_1990   ESP_013076_1990   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.75

203.

1.92

-21.6

63.2

63.0

Gullies Previously Identified in MOC Image:   ESP_013849_1080   ESP_013981_1080   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-71.9

354.

-7.6

-22.1

56.8

59.0

Warrego Valles Headwater Region:   ESP_013153_1390   ESP_013298_1390   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.6

266.

-5.4

6.316

42.0

39.7

Chain of Cones and Craters in Isidis Planitia:   ESP_013054_1900   ESP_013199_1900   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.766

83.1

-5.1

9.582

56.5

54.2

Basal Exposure of South Polar Layered Deposits:   ESP_013145_1070   ESP_013277_1070   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-73.0

133.

0.46

-14.5

55.6

56.1

Pits in Hydrae Chasma:   ESP_013033_1730   ESP_013745_1730   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.83

297.

0

14.87

47.8

38.4

Layered Crater Fill Material:   ESP_014017_2085   ESP_022021_2085   (Interval in Earth days: 624)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.99

68.5

0.69

16.01

57.5

64.7

Gullies in Light-Toned Rock:   ESP_012795_1395   ESP_013507_1395   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.2

319.

2.74

16.59

45.9

37.2

Exposure of Layers in South Gale Crater with Possible Sulfates:   ESP_014186_1745   ESP_020410_1745   (Interval in Earth days: 485)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.56

138.

8.10

-13.1

35.2

55.9


  


Page 731 of 896 (8,955 images)