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.

Landforms above Subsurface Radar Observations of South Polar Cap:   ESP_084655_1000   ESP_084971_1000   (Interval in Earth days: 25)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-80.0

208.

-0.0

24.15

65.9

69.1

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

Channels in Warrego Valles:   ESP_084850_1375   ESP_092221_1375   (Interval in Earth days: 575)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-42.2

267.

4.95

-16.5

41.9

46.7

Ring-Mound Landforms on Schiaparelli Crater Floor:   ESP_084635_1760   ESP_084859_1760   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.73

14.8

-10.

26.07

38.9

34.4

Hill on South Polar Layered Deposits:   ESP_084887_0900   ESP_084374_0900   (Interval in Earth days: 40)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-89.7

35.5

29.4

29.44

75.3

68.6

Gully with Possible Bright Deposit:   ESP_084576_1385   ESP_085222_1385   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.2

190.

-4.9

8.917

39.9

45.6

Southern Canyon Wall in East Coprates Chasma:   ESP_084888_1645   ESP_076950_1645   (Interval in Earth days: 618)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.4

305.

13.0

-5.95

33.5

41.3

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

Cratered Cones in Amazonis Planitia:   ESP_084866_2075   ESP_085011_2075   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.42

182.

-3.2

6.99

53.9

51.4

Landforms above Subsurface Radar Observations of South Polar Cap:   ESP_084841_0965   ESP_084815_0965   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-83.2

171.

8.58

-6.10

70.6

71.2


  


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