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.

Flow Ridge in Nereidum Montes:   ESP_085587_1340   ESP_085732_1340   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-45.6

310.

-6.8

16.93

55.1

56.2

Dune Monitoring in North Mid-Latitude Bonestell Crater:   ESP_085388_2220   ESP_085520_2220   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.8

329.

-0.3

-22.8

57.2

57.0

Ridge-Crater Relationships in Osuga Valles:   ESP_085349_1650   ESP_085982_1650   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.7

321.

-4.2

3.855

36.6

42.7

Stepped Features in Tartarus Skopulus:   ESP_085684_1800   ESP_085829_1800   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.074

175.

2.52

26.97

36.6

35.2

Infilled Troughs near Aeolis Planum:   ESP_085553_1800   ESP_085909_1800   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.005

151.

0.99

25.89

36.3

35.9

Alluvial Fans in Kasei Valles:   ESP_085574_2030   ESP_085640_2030   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.67

293.

15.8

1.691

42.0

42.6

Inverted Channel in Noachis Terra:   ESP_085453_1585   ESP_085519_1585   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.1

2.69

9.81

-7.34

38.4

40.4

Transect of Ladon Valles:   ESP_085441_1560   ESP_085507_1560   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.7

330.

9.97

-6.87

39.3

41.3

Margin of Smooth Lobate Deposit in Nereidum Montes:   ESP_085626_1410   ESP_085758_1410   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.8

322.

16.8

-8.36

49.8

53.5

Inverted Channel Noachis Terra:   ESP_085387_1505   ESP_085598_1505   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.1

5.42

6.72

17.19

41.3

43.5


  


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