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.

Terraced Impact Crater on Lobate Debris Apron:   ESP_084759_1385   ESP_084825_1385   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.9

232.

2.14

-19.6

40.6

42.6

Ancient Crust Outcrops at Nectaris Montes:   ESP_084519_1650   ESP_084018_1650   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.7

304.

-17.

-6.83

37.1

40.8

Southeast Aeolis Dorsa Inverted Delta Trunk Channel:   ESP_084854_1735   ESP_084999_1735   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.32

154.

-2.4

9.423

36.0

34.5

Streamlined Features in Granicus Valles:   ESP_084815_2075   ESP_085936_2075   (Interval in Earth days: 87)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.48

133.

7.85

-9.82

54.0

43.9

Landforms above Subsurface Radar Observations of South Polar Cap:   ESP_084674_0970   ESP_084648_0970   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-82.8

55.2

1.85

-13.0

68.4

69.1

Landforms above Subsurface Radar Observations of South Polar Cap:   ESP_084894_1050   ESP_084762_1050   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-75.0

156.

-0.7

14.00

65.3

62.6

Streamlined Features in Hebrus Valles:   ESP_084868_1995   ESP_085567_1995   (Interval in Earth days: 54)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.18

127.

9.06

-7.83

47.5

42.1

Potential Fan Deposit at Head of Mawrth Vallis:   ESP_084715_1990   ESP_085005_1990   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.91

346.

-0.5

15.83

49.8

45.3

Overlapping Debris Aprons within Ganges Chasma:   ESP_084848_1720   ESP_085138_1720   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.01

318.

-8.1

20.34

36.1

33.3

Terminus of Fissure in Athabasca Valles:   ESP_084867_1900   ESP_085078_1900   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.761

156.

0.88

-9.17

42.3

41.1


  


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