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.

Arc of Cones with Summit Pits in CTX Image:   ESP_019577_1970   ESP_019867_1970   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.74

198.

-19.

12.17

53.6

52.8

Diverse Bedrock Exposures on Floor of Nili Patera:   ESP_019595_1890   ESP_019740_1890   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.085

67.0

-15.

1.288

53.9

53.1

Western Edge of Hellas Planitia:   ESP_019596_1365   ESP_020084_1365   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.2

44.5

8.05

-14.8

73.1

68.8

Rayed Crater in Arcadia Region in Themis V35985012:   ESP_019590_2265   ESP_020078_2265   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
46.31

197.

-0.0

-17.7

56.8

65.6

Monitoring of Pits and Fractures in Deuteronilus Mensae:   ESP_019504_2240   ESP_019570_2240   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.81

25.2

1.42

-13.1

54.7

56.8

Ismenius Cavus:   ESP_019333_2140   ESP_019478_2140   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.77

16.9

-14.

-2.15

51.9

52.3

Rocky Central Structure of a Large 40-Kilometer Diameter Crater:   ESP_019441_1595   ESP_019942_1595   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.2

314.

-5.7

23.31

62.9

57.7

Alpine Glacier:   ESP_019213_2210   ESP_019503_2210   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.86

51.3

-8.0

14.46

51.2

52.7

Gemina Lingula Scarp with Outcrop of Layered Deposits and Unconformities:   ESP_018844_2605   ESP_019081_2605   (Interval in Earth days: 19)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.37

27.0

1.70

16.54

62.6

64.5

Steep North Polar Boundary Scarp:   ESP_018928_2640   ESP_019034_2640   (Interval in Earth days: 8)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
83.79

237.

7.24

-7.09

65.4

67.3


  


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