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.

Alluvial Fans and Terraced Scarps in Kasei Valles:   ESP_088541_2025   ESP_088330_2025   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.38

291.

-19.

-6.13

47.7

46.0

North Polar Layered Deposits Structural Geology in Icy Layers:   ESP_088733_2630   ESP_088562_2630   (Interval in Earth days: 13)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
82.71

56.5

6.65

-7.41

59.1

59.3

Steep Sandy Slopes in Coprates Chasma:   ESP_088554_1660   ESP_088620_1660   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.7

298.

11.2

-14.2

63.4

65.0

Ridged Flow-Like Features in Deuteronilus Mensae:   ESP_088445_2225   ESP_088511_2225   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.33

26.8

8.67

-8.24

42.8

44.5

Stereo for Kunowsky Crater Dunefield:   ESP_088644_2370   ESP_088420_2370   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
56.72

350.

5.32

-16.7

46.6

47.9

Layering and Contact in Lucus Planum:   ESP_088545_1725   ESP_088756_1725   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.43

184.

-3.0

-16.9

60.3

61.4

Dunes in Northern Mid-Latitude Crater:   ESP_088469_2410   ESP_088548_2410   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
60.69

87.7

5.29

19.86

47.3

46.3

A Fissure and Channel near Pavonis Mons:   ESP_086934_1775   ESP_087435_1775   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.54

247.

-7.1

24.56

49.0

51.0

Ring-Shaped Mounds in Ceraunius :   ESP_086815_2115   ESP_087092_2115   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
31.79

249.

16.7

-7.37

40.6

42.5

Dune Survey:   ESP_088162_2540   ESP_088676_2540   (Interval in Earth days: 41)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
73.92

186.

-0.7

14.11

53.6

53.3


  


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