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.

Basal Unit and Dunes:   PSP_009913_2635   PSP_010019_2635   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
83.51

118.

8.64

-5.81

63.1

64.9

Basal Unit and North Polar Layered Deposits in Chasma Boreale Scarp:   PSP_009995_2650   PSP_010128_2650   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
85.06

0.70

19.4

5.177

65.3

66.6

Eroding Margin of Low Latitude North Polar Layered Deposits:   PSP_009938_2640   PSP_010176_2640   (Interval in Earth days: 19)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
83.87

139.

19.6

5.57

63.3

66.3

Possible Pingos in Gusev Crater:   PSP_009385_1655   PSP_009886_1655   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.2

175.

-18.

5.226

65.1

63.0

High-Latitude Exposure of North Polar Layered Deposits:   PSP_009352_2680   PSP_009618_2680   (Interval in Earth days: 20)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.98

258.

-6.4

-18.5

63.9

65.0

Possible Intravalley Paleolake in Shalbatana Vallis:   PSP_009683_1830   PSP_010316_1830   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.989

316.

-5.0

-21.7

54.6

56.7

Aprons with Channels in Eos Chasma:   PSP_009327_1665   PSP_009960_1665   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.3

317.

0

-20.9

63.3

64.2

Alcove with Bright Rocky Slope Streaks:   PSP_009762_1905   PSP_009907_1905   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.40

318.

-0.3

15.26

51.2

50.3

Interaction of Cratered Cone and Crater Ejecta:   PSP_009906_2225   PSP_010196_2225   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.33

343.

-7.7

14.62

48.0

48.7

Multiple Unconformities in the Upper North Polar Layered Deposits:   PSP_010181_2600   PSP_010234_2600   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.74

23.4

-6.9

-18.7

64.6

66.2


  


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