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.

Features around Crater in Arabia Terra:   ESP_089500_2200   ESP_089645_2200   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.86

26.3

-20.

-9.09

51.3

51.6

Mamers Valles:   ESP_089329_2175   ESP_089606_2175   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.21

13.9

-10.

-29.1

48.8

52.9

Planned ExoMars Landing Ellipse Imaging in Oxia Planum:   ESP_089581_1995   ESP_089291_1995   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.24

335.

3.28

-24.9

50.3

51.5

Exposure of North Polar Layered Deposits:   ESP_089303_2605   ESP_089962_2605   (Interval in Earth days: 52)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.27

345.

0.31

14.90

62.1

69.6

Low Shield Summit Vent in Syria Planum:   ESP_089307_1635   ESP_089452_1635   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-16.2

260.

-0.1

16.18

64.9

63.4

Sample of Scalloped Terrain West of Erebus Montes:   ESP_089349_2195   ESP_089072_2195   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.37

187.

-8.3

14.20

48.9

44.9

Potential Compound Dune:   ESP_089573_2610   ESP_089389_2610   (Interval in Earth days: 14)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.87

160.

19.2

-5.86

64.3

63.7

Dune Interaction with Residual Polar Ice:   ESP_089273_2595   ESP_089365_2595   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.28

88.0

-3.9

11.81

61.5

61.4

Light-Toned Deposits in Iani Chaos:   ESP_089383_1780   ESP_089871_1780   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.75

341.

18.5

-11.7

55.6

57.9

Large Crater on Slope of Layered Deposits:   ESP_089517_1735   ESP_089095_1735   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.23

287.

-20.

-5.59

60.6

59.8


  


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