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.

Dune Interaction with Residual Polar Ice:   ESP_080121_2605   ESP_079673_2605   (Interval in Earth days: 35)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.53

98.1

23.9

9.047

58.0

57.0

Dune Interaction with Residual Polar Ice:   ESP_080069_2605   ESP_080583_2610   (Interval in Earth days: 40)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.66

98.6

-8.3

6.294

59.7

63.1

Preserved Meanders in Jezero Crater Outlet:   ESP_079846_1990   ESP_079701_1990   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.72

78.4

29.1

12.20

46.0

47.2

Olympia Cavi Interior Scarps and Dunes:   ESP_079958_2650   ESP_080076_2650   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
85.06

235.

-7.8

6.723

61.6

61.6

Erosional Features on Olympus Mons:   ESP_080078_2075   ESP_080144_2075   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.31

226.

8.64

-7.86

46.4

48.0

Defrosting Dunes in Chasma Boreale:   ESP_080112_2645   ESP_080139_2645   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.55

336.

8.30

-5.70

61.4

62.2

Potential Fluvial Ripples on Surface above Shalbatana Vallis:   ESP_079811_1875   ESP_079877_1875   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.589

318.

-2.2

-21.2

53.2

54.8

North Polar Residual Cap Topography:   ESP_079851_2680   ESP_079734_2680   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.82

241.

-8.4

-22.5

63.2

63.4

Equatorial-Facing Trough Slope Exposure of North Polar Layered Deposits:   ESP_079448_2670   ESP_079515_2670   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
86.93

101.

-6.8

-20.7

61.8

62.5

Hillslope-Channel Coupling in High Drainage Density Region:   ESP_079633_1610   ESP_079000_1610   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.7

141.

-8.3

2.535

68.6

65.7


  


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