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.

Western Rim of Well-Preserved Impact Crater :   ESP_028568_2130   ESP_032893_2130   (Interval in Earth days: 337)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.60

253.

6.82

-6.33

53.8

45.3

Layers in Northern Meridiani Planum :   ESP_028340_1865   ESP_060001_1865   (Interval in Earth days: 2467)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.308

1.62

5.28

-12.5

51.8

38.1

Ridges and Troughs in Crater East of Hellas Planitia :   ESP_028402_1455   ESP_028468_1455   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.2

114.

7.97

-9.94

67.6

68.2

Rounded Deposit with Light Toned Layers :   ESP_028298_2105   ESP_033414_2105   (Interval in Earth days: 399)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
30.15

65.8

-4.3

25.99

51.3

38.5

Ridge in Eos Chasma :   ESP_028342_1635   ESP_034302_1635   (Interval in Earth days: 465)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-16.5

310.

-0.3

18.00

59.8

56.3

Layered Bedrock in Gusev Crater :   ESP_028492_1645   ESP_033819_1645   (Interval in Earth days: 415)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.1

175.

-6.9

16.51

59.0

49.8

Source Region of Harmakhis Vallis :   ESP_028561_1410   ESP_028983_1410   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.5

94.3

7.74

-8.03

68.4

64.7

Star and Barchan Dune Changes :   ESP_028416_1710   ESP_033519_1710   (Interval in Earth days: 398)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.74

89.0

2.64

-25.2

56.2

45.7

Well-Preserved Impact Crater on Alba Patera :   ESP_028410_2170   ESP_028766_2170   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.72

247.

-8.1

1.304

54.1

58.0

Layered Deposits in Small Crater in Terra Cimmeria :   ESP_028547_1405   ESP_037276_1405   (Interval in Earth days: 681)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.9

118.

-7.8

19.54

69.8

70.3


  


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