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_073960_1630   ESP_074105_1630   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-16.6

211.

-5.2

10.88

53.8

51.2

Chryse Chaos:   ESP_074114_1860   ESP_073969_1860   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.991

323.

8.91

-5.81

57.9

59.3

Channel Crossing Heavily Eroded Wrinkle Ridge:   ESP_074146_1485   ESP_073790_1485   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.4

175.

-4.9

-20.8

51.1

57.1

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

Inlet Valley to Jezero Crater:   ESP_074268_1990   ESP_074413_1990   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.58

76.8

6.94

20.62

63.9

62.7

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

Phaethontis Region Slope Monitoring:   ESP_074145_1390   ESP_073868_1390   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.7

204.

-14.

6.12

53.0

55.6

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

Small Delta or Fan:   ESP_073983_1385   ESP_074260_1385   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.3

306.

0.43

-26.6

54.4

52.4


  


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