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.

Ancient Valley Network Adjacent to Low-Albedo Outcrops:   PSP_004832_1310   PSP_005465_1310   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-48.6

294.

6.60

-9.99

40.0

44.9

Complex Banded Terrain of Hellas Floor:   PSP_006555_1395   PSP_007122_1395   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.1

52.6

0

-11.5

55.2

65.2

Study Spider Evolution:   PSP_005513_0950   PSP_005817_0950   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-85.0

95.0

0.87

-16.4

72.9

79.4

Erosional Features and Knob in Argyre Planitia:   PSP_005860_1340   ESP_011424_1340   (Interval in Earth days: 433)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-45.4

308.

3.54

17.72

47.2

66.8

Sinuous Ridge in Dark Lava Flow in Western Elysium Planitia:   PSP_006723_1865   PSP_007013_1865   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.196

140.

-7.6

15.48

37.8

37.9

Central Pit and Chaos of A Lage Impact Crater:   PSP_006908_1470   ESP_020173_1470   (Interval in Earth days: 1034)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.9

132.

8.41

-10.6

55.6

62.9

Large Crater on Edge of South Polar Layered Deposits:   PSP_005575_0995   PSP_005839_0995   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-80.5

189.

-6.9

-21.1

70.3

75.6

Eridania Scopulus:   PSP_006565_1270   ESP_011338_1270   (Interval in Earth days: 372)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-52.7

141.

0

-12.7

64.5

73.4

Impact Flow Features:   PSP_005616_1440   ESP_011536_1440   (Interval in Earth days: 461)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.7

129.

-4.5

21.05

38.9

61.4

Fresh 6-Kilometer Diameter Crater Near Galaxias Mensae:   PSP_005971_2160   ESP_011456_2160   (Interval in Earth days: 428)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.88

147.

1.17

-12.5

52.6

65.4


  


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