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.

Unconformities in North Polar Layered Deposits :   ESP_044408_2650   ESP_044435_2650   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.69

131.

7.80

-6.64

59.7

60.2

Southwest Coprates Chasma Wall Slopes :   ESP_044351_1665   ESP_044839_1665   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.5

293.

7.41

-7.71

59.7

60.0

Western Rim and Ejecta of Fresh 8-Kilometer Crater in Margaritifer Terra :   ESP_044349_1605   ESP_043861_1605   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.2

348.

6.98

27.09

63.7

61.6

Pitted Cones in Utopia Planitia :   ESP_044424_2120   ESP_045268_2120   (Interval in Earth days: 65)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
31.72

95.2

2.15

16.00

39.8

41.3

Exposure of North Polar Layered Deposits :   ESP_044495_2695   ESP_044718_2695   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
89.44

3.84

-28.

-26.0

65.2

65.7

Steep-Sided Hill in Melas Chasma :   ESP_044338_1690   ESP_044826_1690   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.1

289.

-9.4

-23.2

59.1

59.5

Candidate ExoMars Landing Site in Aram Dorsum :   ESP_044217_1880   ESP_051944_1880   (Interval in Earth days: 603)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.009

348.

7.29

27.14

46.7

39.8

Landforms in the Northeast Syrtis Major Region :   ESP_044372_1960   ESP_045559_1960   (Interval in Earth days: 93)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.88

76.3

8.31

-15.4

43.2

46.7

Northern Erg Dunes in Summer :   ESP_044501_2605   ESP_044804_2605   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.15

139.

-5.0

10.34

57.2

57.6

Eos Chasma :   ESP_044403_1625   ESP_052051_1625   (Interval in Earth days: 596)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-17.0

315.

-6.0

-25.3

62.9

58.5


  


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