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.

Glacier-Like Form Terminus into Valley Fill:   ESP_085405_2185   ESP_085748_2185   (Interval in Earth days: 26)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.97

226.

-4.2

-17.4

54.5

51.5

Curved Channel near Crater Rim:   ESP_085495_2165   ESP_085983_2165   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.91

289.

-1.3

-16.0

51.8

48.1

Ridge-Crater Relationships in Osuga Valles:   ESP_085349_1650   ESP_085982_1650   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.7

321.

-4.2

3.855

36.6

42.7

Triangular Faceted Spurs in East Candor Chasma:   ESP_085693_1740   ESP_085838_1740   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.03

291.

-3.9

20.84

37.7

36.9

Alluvial Fans in Kasei Valles:   ESP_085363_2035   ESP_085297_2035   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.14

294.

0.51

16.99

45.1

44.7

North Pole Facing Deposit in Crater:   ESP_085325_2220   ESP_085813_2220   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.70

249.

-2.3

2.947

58.0

51.8

Inverted Channel in Noachis Terra:   ESP_085571_1600   ESP_085782_1600   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.9

23.0

-4.5

12.69

40.3

41.8

Hillslope Shapes on Holden Crater Rim:   ESP_085006_1550   ESP_085151_1550   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.7

325.

2.17

18.92

36.0

35.9

Streamlined Form and Hill in Marte Vallis:   ESP_085156_1980   ESP_085433_1980   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.73

185.

7.29

-6.33

43.5

42.2

Raised Glacier-Like Forms in Arabia Terra:   ESP_085043_2150   ESP_085109_2150   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.67

27.6

6.88

-10.0

56.2

56.3


  


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