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.

South Polar Cap Vertical Change Monitoring :   ESP_057761_0930   ESP_057549_0930   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-86.7

16.3

0.27

14.63

66.8

64.0

Bedforms on Floor of Li Fan Crater :   ESP_057541_1330   ESP_057686_1330   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.8

206.

-1.6

21.88

38.1

36.1

Landslide Scarp and Deposits :   ESP_057853_1835   ESP_057919_1835   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.274

324.

8.90

-5.36

40.4

40.5

South Polar Layered Deposits :   ESP_057835_0915   ESP_057784_0915   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.5

134.

25.0

17.49

66.9

67.6

Erosional Scarp in Mid-Latitude Mantle :   ESP_057571_1245   ESP_057782_1245   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-55.1

109.

0.53

11.93

42.2

41.7

Pit Near Pavonis Mons :   ESP_057592_1840   ESP_057526_1840   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.738

248.

-7.8

8.589

44.8

44.6

Candidate Recent Impact Site :   ESP_057118_1615   ESP_075001_1615   (Interval in Earth days: 1393)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.2

227.

-2.5

9.444

40.1

40.7

Medusae Fossae Layers :   ESP_057344_1680   ESP_057832_1680   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.6

178.

-6.1

13.03

39.8

32.8

Central Pit of 21-Kilometer Diameter Crater in Terra Sabaea :   ESP_057151_1580   ESP_066514_1580   (Interval in Earth days: 730)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.9

47.2

-0.3

-20.4

38.8

41.1

Layering in Burroughs Crater :   ESP_057439_1075   ESP_057241_1075   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-72.3

118.

-3.6

11.83

53.7

53.2


  


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