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.

Layered Terrain between Aeolis and Zephyria Plana:   ESP_020594_1735   ESP_020739_1735   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.38

153.

-1.7

14.49

54.5

52.8

Central Structure of Large Impact Crater:   ESP_020695_1440   ESP_029398_1440   (Interval in Earth days: 678)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.5

280.

-0.9

26.38

56.6

55.8

Possible Carbonate-Rich Terrain in Central Stucture of Leighton Crater:   ESP_020492_1830   ESP_021481_1830   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.023

57.7

-3.5

-19.7

55.7

54.9

Central Peak of an Impact Crater in Promethei Terra:   ESP_020846_1400   ESP_029536_1400   (Interval in Earth days: 677)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.5

118.

1.54

-24.2

55.4

59.0

Ridges in Meridiani Planum:   ESP_020560_1835   ESP_028551_1835   (Interval in Earth days: 623)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.475

0.44

5.90

25.06

55.1

51.1

Crater Fill Deposit:   ESP_020532_1465   ESP_020677_1465   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.1

50.6

-7.0

7.211

58.6

55.7

Material Flowing Through Gap in Crater Rim East of Hellas Planitia:   ESP_020543_1345   ESP_029246_1345   (Interval in Earth days: 678)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-45.2

111.

-0.3

25.69

62.1

61.5

Fresh 3-Kilometer Diameter Rayed Crater on Preexisting Crater Terrace:   ESP_020752_1500   ESP_021596_1500   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.5

163.

0.50

-27.6

54.5

45.8

Terrain between Aureum and Hydaspis Chaos:   ESP_020416_1805   ESP_073151_1805   (Interval in Earth days: 4109)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.240

333.

-6.3

3.415

55.6

57.2

Ejecta of Very Well-Preserved Crater:   ESP_020723_2235   ESP_064845_2235   (Interval in Earth days: 3438)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.26

225.

-4.6

28.28

72.1

71.8


  


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