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.

Possible Kaolin-Rich Terrain in Central Peak:   ESP_060394_1720   ESP_060750_1720   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.67

73.6

-0.5

19.34

46.8

49.2

Sand Dune Changes in Hellespontus Region:   ESP_060224_1350   ESP_060290_1350   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-44.8

38.7

7.87

-8.66

69.3

71.1

Bright Slope Streaks in Arabia Terra:   ESP_060408_1985   ESP_060342_1985   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.29

48.9

-8.2

11.45

38.6

36.6

Ridges and Alcoves:   ESP_060238_1820   ESP_060805_1820   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.070

11.2

-1.5

16.93

40.6

44.5

Sinuous Gullies and Arcuate Ridges:   ESP_060214_1355   ESP_060280_1355   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-44.1

311.

8.88

-7.81

68.5

70.4

Erosion within Cerberus Fossae:   ESP_060259_1905   ESP_053652_1905   (Interval in Earth days: 514)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.24

157.

-4.3

5.709

38.6

46.7

Eastern Edge of Polar Cap Outlier in Olympia Mensae:   ESP_060340_2540   ESP_060353_2540   (Interval in Earth days: 1)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
73.96

94.3

-7.8

7.097

61.7

60.8

Light-Toned Deposits along Ius Chasma Wallrock:   ESP_060479_1730   ESP_060835_1730   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.15

273.

-9.0

12.07

48.0

50.2

Ridged Landforms in Noachis Terra South of Greeley Crater:   ESP_060344_1360   ESP_086363_1360   (Interval in Earth days: 2027)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.5

3.73

-2.7

-12.5

70.6

66.9

Pitted Cones in Chryse Planitia:   ESP_060490_2170   ESP_060846_2170   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.71

327.

-1.8

13.14

40.0

38.3


  


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