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.

Faulted Plains in Tempe Terra:   ESP_027842_2250   ESP_028198_2250   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.42

272.

-6.0

8.621

49.1

52.1

Arabia Terra Sample:   ESP_027971_1905   ESP_030239_1905   (Interval in Earth days: 176)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.17

354.

-0.9

10.96

50.3

56.5

Layered Bedrock on Crater Floor:   ESP_028074_1605   ESP_028918_1605   (Interval in Earth days: 65)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.4

66.2

4.51

-9.37

62.1

58.5

Cratered Cones within a Flow Unit in Grjota Valles:   ESP_027978_1955   ESP_028466_1955   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.18

162.

6.83

-12.0

48.6

52.8

Bouldery Layered Slopes in Noctis Labyrinthus:   ESP_027816_1725   ESP_028515_1725   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.18

267.

6.39

-10.2

56.4

56.5

Variable Relief of North Polar Layered Deposits:   ESP_028182_2650   ESP_028010_2650   (Interval in Earth days: 13)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.84

323.

-3.7

8.258

72.2

69.4

Crater Central Uplift in Solis Planum:   ESP_027987_1565   ESP_036914_1565   (Interval in Earth days: 695)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.2

281.

9.65

-2.23

64.3

66.0

Fractures in Chryse Planitia:   ESP_027959_1990   ESP_028737_1990   (Interval in Earth days: 60)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.71

321.

-5.3

7.285

48.9

53.3

Possible Future Landing Site in Mawrth Vallis:   ESP_028011_2055   ESP_028288_2055   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.33

339.

11.0

-7.26

47.3

51.1

Crater on Lobate Apron:   ESP_028083_2310   ESP_028162_2310   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.88

175.

-23.

-2.19

55.5

54.6


  


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