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.

Embayed Crater in Western Elysium Planitia:   ESP_011720_1835   ESP_012353_1835   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.484

142.

7.82

-9.32

57.5

58.2

Eastern Half of Well-Preserved 7-Kilometer Diameter Gullied Crater:   ESP_012483_1425   ESP_012338_1425   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.2

198.

-5.3

-17.7

50.7

53.8

Unusual and Pristine Crater Morphology:   ESP_011717_1910   ESP_012429_1910   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.63

224.

-6.7

14.06

59.9

59.2

Folded Layered Deposits:   ESP_012305_1865   ESP_012371_1865   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.390

11.8

1.20

-19.8

58.6

60.1

Grand Canyon of Gale Crater:   ESP_012340_1750   ESP_012195_1750   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.18

137.

5.40

-12.9

54.3

56.5

Possible Olivine-Rich Terrain:   ESP_012501_1590   ESP_092215_1590   (Interval in Earth days: 6211)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.8

64.0

0.76

27.93

50.0

43.3

Contact between Wallrock and Light-Toned Rocks in Ophir Chasma:   ESP_011662_1750   ESP_011807_1750   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.76

287.

6.98

23.57

56.8

55.2

Gullies in Crater near Hellas Planitia:   ESP_011948_1335   ESP_012014_1335   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-45.9

45.9

-6.0

-22.2

61.0

61.2

Light-Toned Gully Feature or Mass Movement:   ESP_012417_1435   ESP_012839_1435   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.0

200.

-5.5

-20.8

51.5

46.6

Enigmatic Uplift on the Floor of Echus Chasma:   ESP_011715_1800   ESP_012203_1800   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.05

279.

8.06

-26.2

57.0

58.9


  


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