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.

Light-Toned Layering in Plains South of Melas Chasma :   PSP_002617_1690   PSP_003118_1690   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.0

281.

-0.7

24.63

56.4

52.3

Gullies in Dark Layers in Crater Wall:   PSP_002212_1335   PSP_002291_1335   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.2

184.

-6.7

21.92

73.0

70.0

Exposure of Polar Layered Deposits Not Well Covered by Mars Global Surveyor:   PSP_001342_2680   PSP_001568_2680   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
88.04

62.4

-6.0

-13.1

70.2

72.6

Potential Lobe of Lahar Flow Front:   PSP_002042_2090   PSP_002108_2090   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.85

134.

5.87

-13.1

53.3

55.7

Northern Plains Sample:   PSP_001945_2515   PSP_002077_2515   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
71.07

252.

2.20

-10.6

67.3

70.4

Fresh-Looking Gullies:   PSP_001714_2390   PSP_001846_2390   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
58.73

82.3

3.50

-8.24

57.8

60.7

Dark Central Uplift in an Unnamed Crater in Hesperium Planum:   PSP_002201_1665   ESP_025105_1665   (Interval in Earth days: 1785)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.5

119.

-1.7

-18.5

58.5

51.6

Tooting Crater Interior:   PSP_001538_2035   PSP_002158_2035   (Interval in Earth days: 48)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.18

207.

23.1

11.74

47.1

53.3

Mawrth Vallis Layered Terrain:   PSP_001388_2035   PSP_010183_2035   (Interval in Earth days: 685)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.24

342.

-5.3

8.558

48.9

48.7

Terraced Fan in Memnonia:   PSP_001644_1715   PSP_001842_1715   (Interval in Earth days: 15)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.60

200.

21.0

-7.60

56.5

58.2


  


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