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.

Rocky Mesas in Western Elysium Planitia:   ESP_016889_1885   ESP_017311_1885   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.145

143.

7.82

-11.8

45.3

48.9

Southern Extension of Claritas Fossae:   ESP_016647_1360   ESP_016792_1360   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.7

277.

2.88

16.79

76.6

77.4

Quasi-Periodic Layering in a Large Crater:   ESP_016776_1810   ESP_016921_1810   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.019

351.

-7.5

9.544

49.0

48.8

Lobate Tongue Terminus in CTX Image:   ESP_016418_2255   ESP_017130_2255   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
45.06

38.1

-2.1

10.57

44.3

41.3

Crater West of Niesten Crater:   ESP_016510_1515   ESP_019279_1515   (Interval in Earth days: 216)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.2

56.2

-2.9

14.98

64.0

66.9

Potential Rhythmic Layering in East Gale Crater with Hydrated Signature:   ESP_016375_1750   ESP_016520_1750   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.15

138.

1.01

18.09

48.0

48.2

Small Volcano in Tharsis Region:   ESP_016806_2005   ESP_016872_2005   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.15

247.

16.4

-3.58

40.3

42.2

Interesting Crater Ejecta in Columbus Crater:   ESP_016861_1505   ESP_017639_1505   (Interval in Earth days: 60)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.3

193.

1.16

-12.7

68.3

73.7

Very Recent Small Impact Crater:   ESP_016630_1720   ESP_030291_1720   (Interval in Earth days: 1064)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.08

17.6

-3.5

8.058

52.4

48.4

Terrain South of Newcomb Crater:   ESP_016736_1520   ESP_068970_1525   (Interval in Earth days: 4070)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.6

5.59

4.65

-7.50

65.7

63.9


  


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