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 South Wall of Olympus Mons Caldera:   PSP_007023_1980   PSP_007168_1980   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.81

226.

-0.2

12.29

38.7

38.1

Rayed Crater with Central Peak at Acidalia Planitia-Arabia Terra Boundary:   PSP_007123_2250   ESP_023803_2250   (Interval in Earth days: 1300)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.71

12.7

-0.0

26.95

46.9

54.3

Rocky Central Uplift of 80-Kilometer Diameter Crater:   PSP_007978_2005   ESP_024487_2005   (Interval in Earth days: 1286)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.18

69.4

0

-26.2

42.1

39.4

Unnamed Small Rayed Crater in Hesperia Region:   PSP_008135_1520   PSP_008425_1520   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.9

108.

-4.0

6.037

68.6

70.2

Craters on an Ice-Rich Debris Apron:   PSP_007832_1385   ESP_060736_1385   (Interval in Earth days: 4123)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.3

103.

1.98

-19.2

74.9

74.8

Inverted Channel and Fan Draining into Crater:   PSP_008185_1750   ESP_035032_1750   (Interval in Earth days: 2092)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.17

180.

3.94

-14.1

53.7

56.6

Gullies:   PSP_007456_2140   ESP_016040_2140   (Interval in Earth days: 669)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.74

281.

-4.6

-22.7

41.7

43.6

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

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

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


  


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