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.

Well-Preserved 6-Kilometer Diameter Impact Crater:   ESP_017334_2300   ESP_017413_2300   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
49.67

230.

-12.

9.171

44.2

42.2

Hellas Planitia Terrain:   ESP_017644_1420   ESP_025925_1420   (Interval in Earth days: 645)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.8

56.7

5.17

-12.5

79.0

76.3

Mini-Chaos in Crater Floor:   ESP_017459_1990   ESP_053827_1990   (Interval in Earth days: 2834)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.80

61.3

-4.8

-27.4

44.6

46.9

Impact Crater Exposing Stratigraphy in Eos Chasma:   ESP_017463_1630   ESP_018241_1630   (Interval in Earth days: 60)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-16.6

315.

4.08

-7.28

63.1

65.0

Gullied Crater Wall in Noachis Terra:   ESP_017594_1430   ESP_062903_1430   (Interval in Earth days: 3530)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.5

341.

5.18

-5.34

77.9

76.3

Central Uplift of an Impact Crater:   ESP_017603_1550   ESP_026095_1550   (Interval in Earth days: 661)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.7

94.5

2.99

-24.4

69.4

68.6

Lava Delta in Eastern Tharsis Region:   ESP_017307_2050   ESP_017729_2050   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.97

249.

4.76

-11.9

41.7

44.1

Layering Exposed in Crater Walls:   ESP_017382_1825   ESP_028063_1825   (Interval in Earth days: 833)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.570

5.14

0.74

-11.5

51.1

53.6

Hanging Valley and Terraces in Mangala Valles:   ESP_017691_1735   ESP_017902_1735   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.18

209.

6.65

-2.54

56.9

57.9

Bacolor Crater Gullies:   ESP_017681_2135   ESP_017971_2135   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.97

118.

-8.0

14.61

42.4

41.1


  


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