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.

Possible MSL Rover Landing Site Holden Crater:   ESP_019045_1530   ESP_019322_1530   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.6

325.

8.87

-19.8

67.8

68.0

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

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

Gemina Lingula Scarp with Outcrop of Layered Deposits and Unconformities:   ESP_018844_2605   ESP_019081_2605   (Interval in Earth days: 19)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.37

27.0

1.70

16.54

62.6

64.5

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

Layered Terrain in Aeolis Planum:   ESP_018959_1730   ESP_019025_1730   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.90

150.

4.52

-18.8

57.2

58.8

Scarp:   ESP_019047_2640   ESP_019298_2640   (Interval in Earth days: 20)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
83.88

235.

0.05

-12.8

67.1

71.2

Crater and Landslides:   ESP_019014_1625   ESP_020214_1625   (Interval in Earth days: 93)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-17.2

89.9

13.9

1.055

62.0

56.9

Floor of Ius Chasma:   ESP_018928_1725   ESP_019350_1725   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.56

277.

-0.3

-16.9

58.0

58.4


  


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