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.

Alluvial Fans in Kasei Valles:   ESP_085574_2030   ESP_085640_2030   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.67

293.

15.8

1.691

42.0

42.6

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

Landforms above Subsurface Radar Observations of South Polar Cap:   ESP_085526_1000   ESP_085513_1000   (Interval in Earth days: 1)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-79.7

185.

8.77

-3.25

79.0

79.5

Xanthe Dorsa:   ESP_085335_2125   ESP_085480_2125   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.46

337.

-1.4

19.20

51.4

48.4

Fissure in Athabasca Valles:   ESP_085500_1900   ESP_085711_1900   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.733

156.

1.29

15.59

38.1

36.6

Margin of Smooth Lobate Deposit in Nereidum Montes:   ESP_085626_1410   ESP_085758_1410   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.8

322.

16.8

-8.36

49.8

53.5

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

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

Pitted Cones near Crater:   ESP_085515_2060   ESP_085449_2060   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.75

105.

1.87

16.40

45.1

44.7

Large Isolated Landform at Chryse Planitia Margin:   ESP_085402_1945   ESP_085547_1945   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.22

310.

5.37

29.46

39.9

37.2


  


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