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.

Gullies as Seen in MOC Image M02-02681:   PSP_007213_1400   ESP_042618_1400   (Interval in Earth days: 2759)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.6

86.3

2.71

26.46

65.4

65.6

Wrinkle Ridge in Hesperia Planum:   PSP_007726_1560   PSP_008082_1560   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.9

115.

8.10

-3.05

61.0

65.3

Hellas Planitia:   PSP_007781_1410   PSP_008137_1410   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.4

55.7

6.07

-3.19

72.0

76.2

Sinuous Ridge in Aeolis Region:   PSP_007395_1775   ESP_016414_1775   (Interval in Earth days: 703)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.46

151.

8.20

27.01

44.8

45.0

Mangala Valles:   PSP_008118_1645   PSP_008408_1645   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.5

210.

4.85

15.67

59.6

61.0

Thermally-Distinct Ridges Seen in THEMIS Images I09390002 and V24116005:   PSP_007838_1555   PSP_008840_1555   (Interval in Earth days: 78)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.0

297.

3.49

-19.3

62.6

70.9

Interaction between Unnamed Crater Ejecta and Pre-Exsisting Terrain:   PSP_007681_2000   PSP_008406_2000   (Interval in Earth days: 57)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.66

259.

-6.6

23.65

41.5

41.9

Complex Banded Flow Terrain on Hellas Basin Floor:   PSP_007702_1405   PSP_008559_1405   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.2

53.5

1.51

-17.5

71.9

80.6

Central Peak and South Rim of Large Fresh Crater in Isidis Basin:   PSP_007107_1900   PSP_009823_1900   (Interval in Earth days: 211)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.02

94.3

0.07

-12.8

39.2

52.4

Inverted Channel and Fan Draining into Crater:   PSP_008185_1750   ESP_035032_1750   (Interval in Earth days: 2092)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.17

180.

3.94

-14.1

53.7

56.6


  


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