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.

North Polar Sand Dunes :   ESP_044199_2565   ESP_044740_2565   (Interval in Earth days: 42)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
76.58

102.

5.08

-14.3

53.9

56.5

Candidate Landing Site for 2020 Mission in Nili Fossae :   ESP_043963_2020   ESP_043818_2020   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.87

78.6

28.7

13.85

38.8

40.0

Well-Preserved 5-Kilometer Impact Crater North of Gale Crater :   ESP_044106_1800   ESP_053679_1800   (Interval in Earth days: 746)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.147

139.

5.54

20.38

50.9

50.5

Rocky Terrain Near Nili Fossae :   ESP_044095_2010   ESP_044662_2010   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.82

77.5

6.46

26.09

41.3

40.2

Candidate ExoMars Landing Site in Oxia Palus Region :   ESP_044178_1985   ESP_061136_1985   (Interval in Earth days: 1322)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.46

335.

-25.

-3.40

44.9

41.7

Ejecta Deposits of Bakhuysen Crater :   ESP_043926_1555   ESP_043781_1555   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.3

16.5

8.94

-9.90

66.6

67.1

Candidate Landing Site for 2020 Mission in Melas Chasma :   ESP_044180_1700   ESP_044325_1700   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.80

283.

-24.

-4.34

59.1

57.9

Eastern Discontinuous Ejecta and Rays of Tomini Crater :   ESP_044146_1965   ESP_043790_1965   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.22

126.

3.15

-13.6

43.2

43.9

Mesa with Ciruclar and Arcuate Scarp Elements :   ESP_044114_2315   ESP_044734_2315   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
51.21

274.

1.21

-28.9

41.7

45.8

Channel Entering Crater in Sirenum Fossae :   ESP_044156_1560   ESP_044512_1560   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.6

220.

-23.

-2.85

68.4

67.3


  


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