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.

Slope Streaks Beginning at Stratigraphic Layers:   PSP_007473_1850   PSP_008264_1850   (Interval in Earth days: 62)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.996

181.

-5.4

5.46

43.6

48.7

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

Possible Chloride Salt Deposit:   PSP_007058_1745   ESP_016354_1745   (Interval in Earth days: 724)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.62

353.

4.05

-22.5

42.7

49.8

Circular Feature with Layers of Repeated Thickness and Expression:   PSP_007427_1820   PSP_007862_1820   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.331

357.

-0.1

20.72

44.2

46.5

Western Elysium Planitia Boundary:   PSP_008015_1840   PSP_009940_1840   (Interval in Earth days: 150)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.067

141.

-0.4

-16.9

47.9

55.3

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

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

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

Recent Crater:   PSP_007750_1900   ESP_051001_1895   (Interval in Earth days: 3370)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.637

176.

5.67

-4.50

43.3

35.5


  


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