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.

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

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

Small Shield in Tharsis Region Embayed by Younger Lavas:   ESP_027988_2010   ESP_033658_2010   (Interval in Earth days: 442)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.48

248.

5.19

-6.24

47.9

39.0

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

Scoured Crater Floor Adjacent to Fan-Shaped Form:   ESP_028037_2140   ESP_033918_2140   (Interval in Earth days: 458)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.48

349.

0.97

-13.3

48.7

41.7

Central Uplift of Crater in Lunae Planum:   ESP_028092_1975   ESP_037309_1975   (Interval in Earth days: 718)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.38

291.

-7.8

6.232

50.0

53.4

Fan in Crater West of Gale Crater:   ESP_027900_1745   ESP_045570_1745   (Interval in Earth days: 1377)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.45

136.

-16.

14.60

57.1

51.7

Possible Noachian Phyllosilicate with Low-Ca Pyroxene Near Nili Fossae:   ESP_027955_2020   ESP_028311_2020   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.63

70.4

-4.7

13.27

48.4

49.4


  


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