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.

Fresh Crater:   ESP_084505_1405   ESP_085217_1405   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.3

328.

7.64

-3.64

37.9

45.2

Gullies on Lobate Flow Feature Basin in Nereidum Montes:   ESP_084532_1335   ESP_084967_1335   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.1

311.

13.9

23.63

40.7

44.2

Crater with Layered Deposit in Western Utopia Planitia:   ESP_084566_2240   ESP_093031_2240   (Interval in Earth days: 660)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.82

91.7

2.57

21.98

70.3

73.6

Craters along Nanedi Valles:   ESP_084835_1860   ESP_092008_1860   (Interval in Earth days: 559)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.788

310.

3.92

28.82

40.3

54.9

Valley in Newton Crater:   ESP_084892_1375   ESP_085591_1375   (Interval in Earth days: 54)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-42.3

201.

-4.8

-16.4

43.0

53.6

Exposed Crater Wall Strata in Oxia Planum:   ESP_084610_1965   ESP_085533_1965   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.27

334.

-4.0

7.925

49.6

39.9

Ridges on Crater Floor in Terra Sabaea:   ESP_084779_1510   ESP_085069_1510   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.6

44.1

6.57

26.75

35.6

36.0

Potential Fan Deposit at Head of Mawrth Vallis:   ESP_084715_1990   ESP_085005_1990   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.91

346.

-0.5

15.83

49.8

45.3

Gullied Crater Wall:   ESP_084670_1435   ESP_085593_1435   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.9

142.

2.83

23.40

37.7

47.0

Yardangs near Scour Pit Field in Medusae Fossae Formation:   ESP_084760_1730   ESP_085050_1730   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.94

200.

-2.4

19.25

36.3

33.6


  


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