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.

Diverse Lithologies in Central Uplift of Stokes Crater:   ESP_019380_2360   ESP_019604_2360   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
55.59

171.

-16.

10.82

58.7

59.7

Flow Material in Equatorial Crater:   ESP_019267_1720   ESP_024858_1720   (Interval in Earth days: 436)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.05

23.2

-8.4

-26.9

58.1

46.5

Crater in Sinus Sabaeus Region:   ESP_019386_1700   ESP_020019_1700   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.0

13.6

3.93

-10.0

57.8

57.1

Bedrock in Walls of Well-Preserved Impact Crater in Tartarus Montes:   ESP_019222_2055   ESP_019367_2055   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.03

167.

-7.6

5.969

49.8

49.8

Bedrock in Hydrae Chasma:   ESP_019336_1730   ESP_019969_1730   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.75

297.

8.78

-6.40

56.2

56.2

Excellent Megabreccia Outcrops along the Walls of Nili Fossae:   ESP_019476_2005   ESP_019621_2005   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.23

73.7

-7.1

8.669

51.7

51.4

Light-Toned Unit along Coprates Region Ridge:   ESP_019468_1670   ESP_019534_1670   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.0

295.

5.62

-17.3

58.7

60.1

North Polar Residual Cap:   ESP_019282_2675   ESP_019257_2675   (Interval in Earth days: 1)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.69

274.

-8.5

-21.6

73.4

73.5

Distal Margins of the Western Ejecta of Corinto Crater:   ESP_019579_1970   ESP_019935_1970   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.91

141.

0.39

12.99

51.8

53.3

Central Uplift in Baldet Crater:   ESP_019529_2030   ESP_025120_2030   (Interval in Earth days: 435)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.68

65.6

1.83

-17.0

51.3

39.8


  


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