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.

Breached Impact Crater in Elysium Planitia:   PSP_004151_1810   ESP_020963_1810   (Interval in Earth days: 1310)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.869

160.

1.37

-21.1

50.9

56.5

Gullies in Southern Latitude Crater:   PSP_004145_1455   ESP_013098_1455   (Interval in Earth days: 698)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.3

329.

-0.1

-21.4

42.1

43.2

Gullies in Small Crater within Kaiser Crater:   PSP_003418_1335   PSP_003708_1335   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.0

18.8

1.32

23.79

54.6

48.4

Lobate Deposit and Mesa Near Reull Vallis:   PSP_003217_1355   ESP_046890_1355   (Interval in Earth days: 3403)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-44.3

105.

7.75

-8.47

56.9

61.5

Gullies in the North-Facing Wall of a Crater:   PSP_003215_1405   PSP_003492_1405   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.9

160.

-6.5

-26.6

56.4

54.0

Dark Materials on Block in Olympus Mons Aureole:   PSP_003806_1975   ESP_012627_1975   (Interval in Earth days: 687)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.32

217.

2.81

19.24

61.8

61.8

Light-Toned Outcrops in the Plains Between Melas and Candor Chasma:   PSP_004318_1730   PSP_004740_1730   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.84

282.

-3.1

-15.3

45.8

41.7

Mangala Valles Cataract:   PSP_003991_1645   PSP_004347_1645   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.3

210.

0

10.73

46.2

41.2

Unnamed Well-Preserved Crater within the Isidis Basin:   PSP_003560_1900   PSP_005828_1900   (Interval in Earth days: 177)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.16

94.5

0.61

10.89

58.6

37.6

Odd Layered and Eroding Crater Fill in Deeply Eroded Craters:   PSP_003773_1630   PSP_003918_1630   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-16.8

42.7

1.82

18.06

48.1

45.3


  


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