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.

Sample Gigas Fossae:   PSP_003410_1840   PSP_003832_1840   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.778

230.

7.27

-6.05

55.8

55.2

Pit Crater Chain in Cutting Lava Flow in Southwest Alba Patera:   PSP_003515_2155   PSP_004359_2155   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.08

240.

-1.9

-21.1

71.8

72.8

Fault in South Polar Layered Deposits:   PSP_004218_1070   PSP_005194_1070   (Interval in Earth days: 76)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-73.0

146.

-2.0

-23.4

56.0

60.0

Mangala Source:   PSP_003635_1615   PSP_005613_1615   (Interval in Earth days: 154)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.2

210.

-1.4

-22.8

49.5

34.9

Western Region of Zunil Crater:   PSP_004309_1880   ESP_020211_1880   (Interval in Earth days: 1239)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.728

166.

4.71

29.29

53.0

52.5

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 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

Gullies in Crater in South Aonia Terra :   PSP_003698_1295   ESP_014009_1295   (Interval in Earth days: 804)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-50.0

294.

5.99

23.69

51.1

41.4

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


  


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