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.

Canyon Walls in Coprates Chasma:   ESP_088646_1655   ESP_088857_1655   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.1

306.

4.01

-9.22

64.2

64.9

A Fissure and Channel near Pavonis Mons:   ESP_086934_1775   ESP_087435_1775   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.54

247.

-7.1

24.56

49.0

51.0

Ring-Shaped Mounds in Ceraunius :   ESP_086815_2115   ESP_087092_2115   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
31.79

249.

16.7

-7.37

40.6

42.5

Dune Monitoring in Northern Mid-Latitude Crater:   ESP_088230_2400   ESP_088454_2400   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
59.81

135.

-4.2

14.96

47.5

46.2

Dune Survey:   ESP_088162_2540   ESP_088676_2540   (Interval in Earth days: 41)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
73.92

186.

-0.7

14.11

53.6

53.3

Dune Monitoring in North Mid-Latitude Crater:   ESP_088261_2420   ESP_088182_2420   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
61.94

6.66

6.67

-7.68

47.4

48.6

Patterned Ground in Elysium Planitia:   ESP_088335_1845   ESP_088546_1845   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.634

156.

3.81

-11.4

52.6

54.2

Dune Field:   ESP_088070_2535   ESP_088413_2535   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
73.41

178.

0.65

-15.8

53.4

54.6

Dune Survey:   ESP_088329_2415   ESP_088817_2415   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
61.26

311.

-0.1

-21.9

47.8

51.3

Candidate ExoMars Landing Site in Oxia Planum:   ESP_088078_2000   ESP_088012_2000   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.56

334.

-28.

-7.03

48.3

46.2


  


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