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.

Exposure of North Polar Layered Deposits:   ESP_019283_2675   ESP_018978_2675   (Interval in Earth days: 24)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.36

264.

-12.

0

73.2

69.5

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

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

Sinuous Ridges with Scroll Bars at a Scarp:   ESP_019328_1750   ESP_019961_1750   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.04

155.

16.6

2.067

54.9

55.3

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

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

Cone Field in Phlegra Dorsa:   ESP_019446_2080   ESP_019591_2080   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.44

172.

-13.

0.751

52.2

52.4

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

Well-Preserved 10-Kilometer Diameter Impact Crater:   ESP_019561_1980   ESP_019917_1980   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.94

272.

6.73

18.70

51.2

52.7

Polar Layered Deposits Unconformity:   ESP_019355_2790   ESP_063517_2790   (Interval in Earth days: 3441)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.70

324.

-5.8

4.781

80.6

80.5


  


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