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.

Steep North-Polar Boundary Scarp:   ESP_018981_2640   ESP_019310_2640   (Interval in Earth days: 26)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
83.81

236.

1.04

17.00

66.3

70.0

Well-Preserved Crater Northeast of Hellas Planitia:   ESP_019120_1585   ESP_027678_1585   (Interval in Earth days: 667)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.2

77.3

3.42

-7.57

64.5

65.6

Central Chasma Boreale Scarp:   ESP_019044_2650   ESP_019360_2650   (Interval in Earth days: 25)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.82

343.

-24.

-14.4

69.4

72.9

Deep Incisions in Mangala Valles:   ESP_018825_1745   ESP_020025_1745   (Interval in Earth days: 93)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.33

209.

0

-15.1

57.0

56.6

Cluster of Zunil Crater Secondaries:   ESP_019064_1835   ESP_019209_1835   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.656

163.

2.92

17.53

52.6

51.6

Steep North Polar Boundary Scarp:   ESP_018863_2650   ESP_019548_2650   (Interval in Earth days: 53)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
85.00

239.

-21.

-7.16

67.1

75.4

Intra-Crater Dunes in Iaxartes Tholus:   ESP_018938_2520   ESP_018925_2520   (Interval in Earth days: 1)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
71.91

344.

17.9

2.43

57.8

58.7

Potential Future Landing Site on North Polar Residual Cap:   ESP_018949_2635   ESP_019067_2635   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
83.53

34.1

-1.6

16.08

65.9

66.5

Banded Massif:   ESP_019094_2255   ESP_019173_2255   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.93

59.7

-8.5

15.76

50.9

49.6

Possible Future Landing Site in Noctis Labyrinthus:   ESP_018955_1730   ESP_019878_1730   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.85

261.

-6.1

8.344

58.0

55.3


  


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