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.

Light-Toned Layering along Plains Adjacent to Melas Chasma:   PSP_005030_1685   ESP_012427_1685   (Interval in Earth days: 576)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.2

284.

3.48

-15.1

35.7

53.6

Basal Exposure of South Polar Layered Deposits:   PSP_005089_1040   PSP_005313_1040   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-75.8

131.

-6.9

7.077

60.1

61.9

Young Double-Layer Ejecta Crater:   PSP_006816_2120   PSP_007027_2120   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
31.47

116.

5.98

-4.03

42.0

41.9

Light-Toned Layering on Plains Next to Ganges Chasma:   PSP_005161_1720   ESP_016237_1720   (Interval in Earth days: 863)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.14

307.

6.27

-10.6

35.3

48.9

Ridges in Nili Fossae Phyllosilicates:   PSP_005855_2020   PSP_006712_2020   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.80

77.1

-2.4

7.233

44.7

38.7

Light-Toned Layering in Plains South of Melas Chasma:   PSP_006230_1690   ESP_012348_1690   (Interval in Earth days: 477)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.8

282.

0

-25.4

35.7

55.3

Fresh Impact Crater:   PSP_005837_1965   PSP_005903_1965   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.41

209.

-7.9

-26.4

42.0

42.9

Fresh Pit Crater on Arsia Mons:   PSP_004913_1735   PSP_005836_1735   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.31

239.

-8.9

1.393

39.5

33.4

Alcove in West Hellas Region:   PSP_006753_1425   PSP_010814_1425   (Interval in Earth days: 317)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.0

45.9

0

-22.6

56.4

72.8

East Candor Region:   PSP_004410_1735   ESP_012229_1735   (Interval in Earth days: 609)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.22

290.

0.51

-28.0

44.7

57.4


  


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