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.

Gullies in Crater North of Iani Chaos:   ESP_026956_1800   ESP_027523_1800   (Interval in Earth days: 45)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.120

345.

-21.

-2.25

54.9

53.7

Northern Plains Cratered Cones in Acidalia Planitia:   ESP_026732_2215   ESP_027431_2215   (Interval in Earth days: 54)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.15

333.

-4.3

-20.7

41.7

46.5

Cones at Edge of North Polar Layered Deposits:   ESP_026905_2610   ESP_027024_2610   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.71

267.

8.70

-5.21

57.0

58.2

Fresh Impact Crater:   ESP_026661_1495   ESP_062977_1490   (Interval in Earth days: 2830)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-30.2

120.

3.50

-8.29

72.9

72.0

Crater Inside Athabasca Valles:   ESP_026620_1880   ESP_026686_1880   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.237

154.

7.94

-13.7

47.9

49.7

Light-Tone Material Crater Wall in CTX Image G02_019002_1586_XN_21S300W:   ESP_026861_1555   ESP_027349_1555   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.0

59.4

5.54

-17.1

68.5

69.1

Very Well-Preserved Impact Crater on Northern Plains:   ESP_026828_2420   ESP_026907_2420   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
61.68

228.

-3.4

13.20

47.2

46.2

Candidate Future Landing Site Near Sabrina Vallis:   ESP_026812_1920   ESP_026878_1920   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.75

313.

-1.3

-21.3

47.4

49.1

Crater on Northern Plains:   ESP_026880_2355   ESP_026959_2355   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
55.32

253.

-20.

-1.45

46.5

45.1

Dunes and North Polar Outlier:   ESP_026634_2595   ESP_026528_2595   (Interval in Earth days: 8)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.16

125.

-21.

5.115

57.5

55.7


  


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