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.

Mesa Stratigraphy at Terby Crater:   ESP_074743_1520   ESP_075376_1520   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.5

73.8

3.18

-17.5

42.8

37.9

Impact-Related Deposits and Flows Northeast of Ascraeus Mons:   ESP_074881_1985   ESP_075382_1985   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.36

260.

-3.6

24.23

61.4

54.4

Mounds and Pits in Residual Ice Cap:   ESP_074884_0930   ESP_074883_0930   (Interval in Earth days: 0)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-86.9

235.

4.93

20.67

65.0

63.6

Small Channel South of Mangala Valles:   ESP_074883_1600   ESP_083059_1600   (Interval in Earth days: 637)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.6

209.

6.85

-7.00

42.0

51.1

Small Ridge near Licus Vallis:   ESP_074741_1775   ESP_074807_1775   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.59

125.

2.84

-23.6

50.1

51.3

Extra-Crater Sinuous Ridge:   ESP_074959_1035   ESP_075434_1035   (Interval in Earth days: 37)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-76.4

308.

4.75

-17.0

57.4

60.1

Channel in Huygens Crater:   ESP_074981_1625   ESP_075192_1625   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-17.2

53.7

6.87

0.528

41.4

39.5

Conical Pit in Residual Ice Cap:   ESP_074910_0925   ESP_074869_0925   (Interval in Earth days: 3)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.5

253.

7.56

25.40

65.2

63.6

Candidate Lake Deposits Fed by Alluvial Fans:   ESP_074827_1655   ESP_073970_1655   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.5

298.

4.36

-6.62

44.2

54.0

Landslide Deposit in West Candor Chasma:   ESP_074867_1730   ESP_067178_1730   (Interval in Earth days: 599)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.82

284.

16.7

-1.45

45.8

39.1


  


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