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.

Lineated Valley Fill in Coloe Fossae:   PSP_008598_2155   PSP_008954_2155   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.16

57.2

-3.6

-18.8

42.2

44.3

Crater Floor Fan:   PSP_008233_1920   PSP_008879_1920   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.72

307.

6.25

-7.44

45.5

49.1

Layers in Uzboi Vallis:   PSP_008338_1525   PSP_010329_1525   (Interval in Earth days: 155)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.4

324.

5.23

-10.4

69.3

70.2

Sinuous Ridge in Aeolis Region:   PSP_007395_1775   ESP_016414_1775   (Interval in Earth days: 703)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.46

151.

8.20

27.01

44.8

45.0

Very Recent Small Crater in Dejnev Crater:   PSP_008145_1545   ESP_027067_1545   (Interval in Earth days: 1474)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.0

195.

-8.7

6.238

66.9

69.0

Well-Exposed Central Uplift in Unnamed Crater:   PSP_007109_1555   ESP_019385_1555   (Interval in Earth days: 956)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.2

43.4

7.44

-4.41

53.1

65.2

Inner Channel Deposit in Kasei Vallis:   PSP_007825_2010   ESP_035463_2010   (Interval in Earth days: 2153)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.84

287.

-3.9

12.13

41.7

43.8

Wall Layers of Tooting Crater:   PSP_007907_2035   ESP_019115_2035   (Interval in Earth days: 873)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.18

208.

-2.3

5.434

41.6

48.0

Reull Vallis:   PSP_007819_1390   PSP_009612_1390   (Interval in Earth days: 140)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.6

99.6

-6.4

7.67

74.7

81.0

Possible Submarine Fan in Eastern Portion of Small Melas Chasma Basin:   PSP_007377_1700   PSP_008379_1700   (Interval in Earth days: 78)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.82

283.

5.56

-6.99

48.4

58.5


  


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