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.

Small Delta or Fan:   ESP_074435_1465   ESP_075292_1465   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.2

205.

-7.5

6.888

47.4

36.9

Steep Southern Coprates Chasma Wall Slopes:   ESP_074392_1655   ESP_074814_1655   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.1

296.

-0.4

-28.8

49.6

47.1

Drainage Divide Migration in Tyrrhena Terra:   ESP_074439_1525   ESP_075296_1525   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.9

94.7

-1.5

13.67

47.1

36.1

Small Delta or Fan:   ESP_074009_1900   ESP_082053_1900   (Interval in Earth days: 626)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.837

310.

-3.3

22.98

60.6

57.3

Gorgonum Chaos:   ESP_074251_1425   ESP_074396_1425   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.9

188.

6.08

18.51

49.3

46.2

Resistant Material in Olympus Mons Aureole Ridges:   ESP_073920_1990   ESP_074065_1990   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.79

218.

1.52

19.57

64.0

63.0

Fossae East of Arsia Mons:   ESP_074262_1720   ESP_074829_1720   (Interval in Earth days: 45)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.74

244.

5.23

-11.8

52.3

47.9

Well-Exposed and Diverse Layered Section of Nirgal Vallis:   ESP_074233_1505   ESP_075235_1505   (Interval in Earth days: 78)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.1

321.

-29.

-5.54

52.0

38.0

Lava-Crater Interaction in Elysium Planitia:   ESP_073949_1860   ESP_074239_1860   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.812

148.

-1.0

25.38

58.9

56.1

Valleys Into Central Pit:   ESP_074253_1825   ESP_074754_1825   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.406

129.

-4.9

6.301

56.8

52.3


  


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