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.

Layered Sinuous Ridge in Argyre Planitia:   ESP_012848_1235   ESP_012782_1235   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-56.2

316.

-7.0

6.567

50.2

50.1

Comparative Gully Morphology:   ESP_013934_1335   ESP_014000_1335   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.0

183.

6.35

-11.3

40.0

41.5

South Polar Layered Deposits Exposed in Promethei Lingula:   ESP_013832_0975   ESP_013647_0975   (Interval in Earth days: 15)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-82.5

112.

-3.5

14.29

64.8

62.0

Light-Toned Outcrops along Ius Region Wallrock:   ESP_012849_1705   ESP_013126_1705   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.22

281.

-3.9

-28.8

49.2

48.0

Small Rayed Crater in Syrtis Major Planum:   ESP_012791_1910   ESP_012857_1910   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.67

62.2

4.22

-17.8

58.5

59.5

Layered Material Exposed on Crater Floor:   ESP_013017_2150   ESP_013518_2150   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.69

8.85

6.51

22.48

72.6

67.8

Layered Alunite-Kaolinite Deposit:   ESP_013775_1490   ESP_021924_1490   (Interval in Earth days: 635)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-30.4

202.

4.83

29.52

34.9

36.8

Gullies:   ESP_012722_1400   ESP_012867_1400   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.6

153.

-6.2

7.111

47.5

44.4

Ejecta of Crater Sectioned by Erosion:   ESP_013362_1710   ESP_013784_1710   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.89

315.

6.60

-9.43

42.6

38.8

Pasteur Crater Mound with Exposed Layers:   ESP_013544_1995   ESP_013610_1995   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.19

24.0

-4.4

-23.3

57.5

57.9


  


Page 744 of 896 (8,955 images)