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.

Layers in Arnus Vallis:   PSP_007187_1925   PSP_010404_1925   (Interval in Earth days: 251)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
12.51

69.9

-2.9

14.53

39.6

51.3

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

Putative Salt Deposits Detected by THEMIS West of Meridiani Region:   PSP_007770_1770   PSP_008917_1770   (Interval in Earth days: 90)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.17

351.

6.87

-11.5

49.0

57.2

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

Lava Flow Contacts in Eastern Elysium Planitia:   PSP_007170_1820   PSP_007381_1820   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.197

174.

13.9

-6.48

40.3

43.9

Gullies in a Crater Wall:   PSP_007977_2385   PSP_008043_2385   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
58.24

89.7

4.13

-8.34

47.7

48.4

Landforms of the Aeolis and Zephyria Regions:   PSP_007606_1785   ESP_016190_1785   (Interval in Earth days: 669)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.38

150.

-1.3

-16.7

47.1

45.8

Possible Sulfates in Coprates Chasma:   PSP_007205_1660   ESP_024505_1660   (Interval in Earth days: 1348)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.9

301.

5.58

-16.3

48.4

44.1

Merging Fretted Terrain Valleys of Coloe Fossae:   PSP_007016_2160   PSP_009956_2160   (Interval in Earth days: 229)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.71

56.4

-8.4

20.49

43.9

45.3

Geometry of Ramparts for Crater in High Southern Latitudes:   PSP_007800_1365   PSP_009593_1365   (Interval in Earth days: 139)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.3

258.

-5.1

7.815

76.5

83.0


  


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