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 Residual Cap:   ESP_080027_2685   ESP_072140_2685   (Interval in Earth days: 615)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
88.45

183.

-27.

-19.8

65.4

73.7

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

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

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

North Polar Residual Cap Topography:   ESP_079914_2695   ESP_079678_2695   (Interval in Earth days: 19)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
89.39

308.

-20.

-22.6

65.0

64.3

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

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

Mid-Erg Dunes in Abalos Undae:   ESP_079970_2615   ESP_079996_2615   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
81.57

279.

-8.8

6.529

59.7

58.9

High-Latitude Icy Terrains:   ESP_079916_2585   ESP_080074_2585   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
78.55

317.

-8.2

6.069

57.8

57.7

Dune Interaction with Residual Polar Ice:   ESP_080175_2590   ESP_080623_2590   (Interval in Earth days: 35)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.01

81.9

1.22

20.21

58.8

61.7


  


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