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.

Streamlined Form North of Mangala Valles:   PSP_007683_1805   PSP_009542_1805   (Interval in Earth days: 145)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.500

207.

-3.0

-16.3

47.1

56.6

Gullies:   PSP_007031_2220   PSP_009826_2220   (Interval in Earth days: 218)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.43

4.84

2.91

18.33

45.6

45.0

Gullies Possibly Produced by Snow or Ice Melting:   PSP_007270_2240   PSP_010487_2240   (Interval in Earth days: 251)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.42

319.

-2.8

11.76

45.5

52.4

Wrinkle Ridge:   PSP_007052_1870   ESP_016361_1870   (Interval in Earth days: 726)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.101

156.

-6.0

26.66

39.8

40.6

Well-Peserved Large Crater with Central Peak and Pit:   PSP_007366_1360   ESP_024732_1360   (Interval in Earth days: 1353)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.4

229.

2.46

-27.4

70.5

67.3

Fresh 7-Kilometer Diameter Crater with Bright Rayed Ejecta:   PSP_007731_2060   ESP_026310_2060   (Interval in Earth days: 1448)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.77

333.

1.95

28.52

40.6

38.7

Well-Exposed Central Uplift in Unnamed Crater:   PSP_007252_1615   ESP_015981_1615   (Interval in Earth days: 680)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.4

98.7

-0.9

-22.0

52.1

52.3

Fresh 10-Kilometer Diameter Unnamed Crater in Terra Sabaea:   PSP_007966_1615   ESP_025055_1615   (Interval in Earth days: 1331)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.1

41.5

5.02

25.73

59.9

51.0

Western Half of Central Peak of Large Well-Preserved Crater:   PSP_007857_1475   PSP_010006_1475   (Interval in Earth days: 168)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.0

140.

-6.7

19.27

68.9

72.7

Mawrth Vallis Outcrops:   PSP_007533_2055   ESP_025466_2055   (Interval in Earth days: 1397)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.21

339.

3.77

-18.9

40.0

40.9


  


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