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.

Eastern Portion of Small Melas Chasma Basin:   ESP_017807_1700   ESP_018875_1700   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.82

283.

-6.2

16.99

60.3

58.1

Sinuous Troughs and Ridges near the Sirenum Fossae:   ESP_017784_1425   ESP_026276_1425   (Interval in Earth days: 661)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.2

193.

11.4

-12.5

78.5

77.9

Layered Terrain in Aeolis and Zephyria Regions:   ESP_017825_1760   ESP_018458_1760   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.75

149.

13.9

-9.22

55.2

57.1

Flow Into Breached Crater in Central Elysium Planitia:   ESP_018062_1810   ESP_018484_1810   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.837

160.

-8.0

-21.3

54.3

55.6

Exposure of Polar Layered Deposits:   ESP_017954_2720   ESP_018111_2720   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
88.19

114.

-9.6

-16.2

63.9

65.3

Light-Toned Outcrops in Noctis Region:   ESP_017979_1715   ESP_018401_1715   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.26

267.

-7.1

-21.7

59.6

60.6

Raised Polygonal Ridges and Light-Toned Material in Syrtis Region:   ESP_018065_1975   ESP_019133_1975   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.49

76.4

-5.2

15.52

46.5

48.0

Ridges and Flow-Like Forms:   ESP_017734_2075   ESP_071880_2075   (Interval in Earth days: 4219)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.32

111.

-1.2

16.1

42.7

47.9

Layered Deposits in Crater in Western Arabia Terra:   ESP_017936_1890   ESP_060489_1890   (Interval in Earth days: 3315)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.810

-0.9

0.22

-9.82

49.5

41.2

Mounds and Polygonal Features in Crater:   ESP_018078_2445   ESP_018210_2445   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
64.31

70.3

10.5

-7.11

48.1

50.0


  


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