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.

Mesa and Mounds in Utopia Planitia :   ESP_047299_2155   ESP_047589_2155   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.08

86.0

3.78

21.88

66.5

67.9

Arcuate Ridges with Gullies :   ESP_047199_1330   ESP_047476_1330   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.5

307.

2.29

-21.6

57.0

54.4

Geryon Montes Wall Landforms :   ESP_047279_1720   ESP_047345_1720   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.74

278.

-1.4

-24.6

50.6

52.2

Stratigraphy along Slope of Layered Deposit in Candor Chasma :   ESP_047371_1740   ESP_055454_1740   (Interval in Earth days: 630)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.82

286.

0

-19.3

50.4

54.5

Steep Terraced Slopes of Impact Crater :   ESP_047370_2090   ESP_083543_2090   (Interval in Earth days: 2819)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.50

309.

-1.9

9.51

64.0

68.8

Landforms in Utopia Planitia :   ESP_047048_2095   ESP_055276_2095   (Interval in Earth days: 641)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
29.24

99.8

5.69

-7.83

60.7

55.8

Lobes and Low-Lying Bakhuysen Crater Ejecta Deposits :   ESP_047170_1580   ESP_047605_1580   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.5

16.4

-7.3

27.91

51.5

44.5

Candidate ExoMars Landing Site in Oxia Palus Region :   ESP_047079_1985   ESP_082830_1985   (Interval in Earth days: 2786)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.48

335.

0.68

19.16

56.9

63.3

North Part of Samara Valles System :   ESP_047145_1660   ESP_047567_1660   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.7

337.

-5.2

-25.7

51.1

50.1

Intersecting Channels near Olympica Fossae:   ESP_045091_2045   ESP_044326_2045   (Interval in Earth days: 59)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.30

249.

-4.6

20.49

42.8

39.4


  


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