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.

Polar Crater with Summer Ice:   PSP_008081_2405   PSP_008793_2405   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
60.34

129.

4.55

-12.0

48.2

47.8

Landforms in Eastern Amazonis Planitia:   PSP_008131_1930   PSP_008421_1930   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
12.68

213.

-6.4

3.766

45.6

46.2

Well-Exposed Scarp of Noachian Phyllosilicates Along Nili Fossae:   PSP_007200_2005   ESP_016153_2005   (Interval in Earth days: 698)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.03

73.6

1.53

26.79

39.1

37.1

Bright Layers in Columbus Crater:   PSP_007710_1500   PSP_008066_1500   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.6

193.

6.36

-4.46

64.8

69.2

Fresh Double-Layered Ejecta Crater:   PSP_007947_2350   PSP_009160_2350   (Interval in Earth days: 95)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
54.48

190.

0.23

-18.0

46.6

47.1

Fine-Branched Ridges:   PSP_007474_1745   ESP_024497_1745   (Interval in Earth days: 1327)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.38

154.

4.28

27.74

47.3

36.8

Crater with Multiple Gully Orientations:   PSP_007001_2200   PSP_007937_2200   (Interval in Earth days: 73)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.48

105.

-8.6

6.751

45.7

41.3

Central Peak Region of Canso Crater:   PSP_007139_2015   ESP_085442_2015   (Interval in Earth days: 6101)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.34

299.

-1.5

-10.2

39.3

44.2

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

Bacolor Crater Interior and Central Peak:   PSP_007106_2135   PSP_009677_2135   (Interval in Earth days: 200)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.99

118.

0.49

-21.5

41.8

47.5


  


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