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.

Contact between Medusae Fossae and Northern Flank of Apollinaris Mons:   ESP_082757_1725   ESP_082322_1725   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.26

173.

6.07

-7.55

55.1

58.2

Spiders with Large Fans:   ESP_082521_0970   ESP_082547_0970   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-82.8

167.

-3.7

11.75

76.5

74.8

Small Group of Dark Dunes in Aurorae Chaos:   ESP_082514_1725   ESP_082725_1725   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.47

330.

-1.2

-26.7

57.0

58.0

Eroded Layered Deposits:   ESP_082864_1555   ESP_075954_1555   (Interval in Earth days: 539)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.3

132.

15.8

-5.7

51.2

35.5

Possible Scour Pits adjacent to Yardangs in Southwest Olympus Mons:   ESP_082597_1890   ESP_082821_1890   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.852

221.

-7.1

26.60

61.0

58.3

Ius Labes Channels:   ESP_082595_1725   ESP_083162_1725   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.39

277.

1.53

-25.7

56.4

54.5

Exposure of Eroded Fan Deposits:   ESP_082858_1655   ESP_082647_1655   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.4

298.

-18.

4.844

54.9

54.9

Impact Crater and Ejecta:   ESP_082677_1910   ESP_083244_1910   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.00

196.

-8.7

-26.0

62.0

62.0

Channels in Nereidum Montes:   ESP_082541_1440   ESP_082607_1440   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.8

315.

2.23

-22.6

57.4

58.5

Uphill Facing Scarps and Lobate Deformation on Slope:   ESP_082523_2085   ESP_082602_2085   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.12

78.9

6.50

29.15

67.2

65.9


  


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