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.

Pitted Cones in Chryse Planitia :   ESP_057866_2125   ESP_058222_2125   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.01

326.

2.17

16.00

61.7

56.2

Mojave Crater Northeastern Rim with Fans and Slope Features :   ESP_057655_1880   ESP_065989_1880   (Interval in Earth days: 650)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.836

327.

9.14

27.23

45.7

54.6

Very Fine Layers along Wall of Collapse Pit in Xanthe Terra :   ESP_057761_1780   ESP_057550_1780   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.07

315.

11.1

-7.28

38.2

41.9

Gullied Crater :   ESP_057700_1415   ESP_058399_1415   (Interval in Earth days: 54)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.2

185.

1.09

-17.6

34.1

37.7

Apollinaris Patera Scarp :   ESP_057753_1720   ESP_057542_1720   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.94

174.

11.1

-7.21

35.3

39.1

Crater on South Polar Layered Deposits :   ESP_057851_0985   ESP_057970_0985   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-81.4

41.3

5.18

-9.26

62.2

64.2

Ice Rich Lobate Deposit Flowing from Crater :   ESP_057524_1425   ESP_057458_1425   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.1

309.

-6.9

6.893

35.4

34.9

Dendritic Ridges in Channel Levees :   ESP_057649_2055   ESP_066458_2055   (Interval in Earth days: 686)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.02

129.

4.17

-14.6

58.6

64.0

South Polar Layered Deposits :   ESP_057680_0920   ESP_057971_0920   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.8

62.6

13.6

8.449

66.0

69.4

Layered Mesas South of Lycus Sulci :   ESP_057646_1900   ESP_067550_1900   (Interval in Earth days: 771)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.872

213.

-1.3

-15.5

47.8

44.2


  


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