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.

Candidate Landing Site for 2020 Mission in Gusev Crater:   ESP_051845_1655   ESP_051911_1655   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.5

175.

14.2

-7.79

52.3

54.3

Lava-Draped Surface in Cerberus Palus:   ESP_051991_1880   ESP_061156_1880   (Interval in Earth days: 714)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.848

147.

2.70

26.28

42.1

43.4

Pit in Upland among Troughs in Western Noctis Labyrinthus Region:   ESP_051829_1755   ESP_063829_1755   (Interval in Earth days: 935)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.36

252.

-0.6

20.12

47.0

55.4

Candidate Red Dragon Landing Site in Arcadia Planitia:   ESP_051857_2210   ESP_051923_2210   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.56

202.

-3.6

-18.3

40.3

41.4

Crater Filled with Ejecta:   ESP_051787_1785   ESP_051286_1785   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.65

317.

11.1

-17.1

44.3

41.4

Lobate Features in Eastern Acidalia Planitia:   ESP_051943_2270   ESP_052088_2270   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
46.83

12.9

0.98

12.26

41.8

40.4

Sinuous Linear Gullies in Hellas Planitia:   ESP_051836_1345   ESP_051770_1345   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-45.3

67.2

-4.7

11.68

75.7

74.0

Outlet Breach in Small Crater:   ESP_051967_1800   ESP_052112_1800   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.102

84.6

-5.4

13.68

46.1

46.0

Cracked Channel-Filling Deposit or Slumped Ejecta:   ESP_051969_2095   ESP_052114_2095   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
29.20

25.8

1.30

16.21

37.9

36.8

Sinuous Ridges and Valleys in Peridier Crater:   ESP_051901_2055   ESP_052046_2055   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.27

83.6

-8.9

6.983

38.6

37.6


  


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