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.

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

Summit of One of Cerberus Tholi :   ESP_044039_1850   ESP_044184_1850   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.872

169.

-2.2

17.44

48.7

47.5

Gullies in Northern Mid-Latitude Crater :   ESP_044122_2335   ESP_051071_2335   (Interval in Earth days: 541)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
52.97

57.4

-8.5

4.472

43.1

51.1

Mini Cinder Cones in Aetheria Region :   ESP_043896_2055   ESP_044885_2055   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.07

110.

-3.2

19.02

40.7

40.2

Streamlined Features and Small Channels adjacent to Ravi Vallis :   ESP_043994_1800   ESP_044139_1800   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.09

318.

-9.2

11.23

51.8

50.7

Channels on Alba Patera :   ESP_044115_2270   ESP_044194_2270   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
46.73

248.

1.66

25.66

40.5

38.4

Nili Patera Dunes :   ESP_043990_1890   ESP_044346_1890   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.769

67.1

-12.

7.288

47.4

46.4

Light-Toned Ridges with Possible Mounds :   ESP_043925_2310   ESP_043635_2310   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.82

31.0

22.7

3.014

39.8

42.2

Pit Near Elysium Mons :   ESP_043974_2090   ESP_078591_2090   (Interval in Earth days: 2698)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.58

139.

6.47

21.08

39.4

41.0

Northern Arabia Terra Deposits :   ESP_044124_2185   ESP_044058_2185   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.21

3.93

2.19

16.92

39.4

38.0


  


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