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.

Mesa in Chryse Planitia:   ESP_071806_2045   ESP_071872_2045   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.20

333.

5.73

-17.1

48.7

51.1

Layers in Meridiani Planum:   ESP_071647_1865   ESP_071792_1865   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.317

358.

-7.7

6.1

54.6

53.3

North Polar Layered Deposits:   ESP_071809_2685   ESP_071531_2685   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
88.70

260.

-28.

-20.7

70.4

67.3

Valley Breaching Gale Crater Rim:   ESP_071642_1735   ESP_071787_1735   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.40

136.

-8.6

6.598

60.5

58.9

Alcove in Melas Chasma Exposing Layers:   ESP_071663_1695   ESP_071808_1695   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.1

283.

-8.7

5.635

62.4

60.9

ExoMars Landing Site within Oxia Planum:   ESP_071951_1980   ESP_071740_1980   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.68

336.

-2.7

14.17

51.3

49.1

North Polar Residual Cap Topography:   ESP_071638_2675   ESP_071798_2675   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.52

194.

-8.4

-27.3

66.8

69.6

Classic Barchans:   ESP_071999_2560   ESP_072157_2560   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
75.79

94.0

-8.0

6.782

64.0

65.1

Potential Channel in Gusev Crater:   ESP_071812_1660   ESP_071891_1660   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.6

175.

-3.7

28.34

63.4

60.8

Dunes with Furrows:   ESP_071736_2575   ESP_071828_2575   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
77.17

75.5

-8.3

7.534

61.8

61.5


  


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