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.

Rayed Crater:   ESP_026937_2145   ESP_027847_2145   (Interval in Earth days: 71)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.12

137.

-0.8

-12.9

41.9

48.3

Possible Future Landing Site in Sabrina Vallis Delta:   ESP_026601_1920   ESP_034605_1920   (Interval in Earth days: 623)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.68

313.

3.61

21.97

46.6

43.1

Exposures of North Polar Layered Deposits with Unconformities:   ESP_026901_2600   ESP_028048_2600   (Interval in Earth days: 90)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.00

23.3

0

15.02

57.0

66.2

Dunes and North Polar Outlier in MOC Image R03-00181:   ESP_026963_2595   ESP_026660_2595   (Interval in Earth days: 24)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.21

124.

13.6

-1.03

56.0

56.1

Well-Preserved Crater with Layered Ejecta on Northern Plains:   ESP_026910_2170   ESP_027477_2170   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.52

155.

-8.4

6.108

42.4

43.9

South Coprates Chasma Dune Changes:   ESP_026905_1660   ESP_027182_1660   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.0

296.

6.57

-16.4

61.6

62.9

Possible Future Landing Site in Mawrth Vallis:   ESP_026600_2060   ESP_034736_2060   (Interval in Earth days: 634)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.53

339.

-0.1

-23.6

42.1

43.7

Cones at Edge of North Polar Layered Deposits:   ESP_026958_2605   ESP_027077_2605   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.62

262.

5.88

-8.25

57.3

58.6

Pits and Channels in Amazonis Planitia:   ESP_026605_2025   ESP_051290_2025   (Interval in Earth days: 1924)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.23

202.

3.69

14.57

42.6

35.3

Possible Phyllosilicates and Fluvial Features Near Hashir Crater:   ESP_026649_1835   ESP_028060_1835   (Interval in Earth days: 109)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.323

84.8

-9.5

13.24

51.7

51.4


  


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