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.

North Polar Erg Changes:   ESP_028055_2605   ESP_028029_2605   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.17

191.

16.3

-0.45

66.3

66.9

Holden Crater Bedform Change Detection:   ESP_028025_1530   ESP_028513_1530   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.5

325.

-0.4

-17.8

66.6

64.6

Possible Prehnite-Bearing Deposits in Northwest Hellas Planitia:   ESP_027903_1535   ESP_026571_1535   (Interval in Earth days: 104)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.2

56.1

-7.1

12.83

67.6

69.4

Faults in Claritas Fossae:   ESP_028199_1535   ESP_028476_1535   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.3

254.

7.56

-10.8

64.9

64.2

Recent Crater on Northern Plains:   ESP_027986_2390   ESP_033933_2390   (Interval in Earth days: 463)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
58.50

297.

3.48

-14.9

54.8

52.3

North Polar Gypsum Dunes:   ESP_027820_2610   ESP_027912_2610   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.93

138.

-6.3

7.587

65.1

65.4

Sinuous Ridge on Crater Wall in Aeolis Region:   ESP_027807_1765   ESP_035112_1765   (Interval in Earth days: 569)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.70

153.

-4.5

12.46

55.5

54.4

Mounds and Small Ridges along Wrinkle Ridge on Huygens Crater Floor:   ESP_027969_1635   ESP_028325_1635   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-16.2

54.6

-23.

-4.61

62.8

60.0

Landforms in Simud Valles in CTX G16_024570_1921_XN_12N038W:   ESP_027814_1940   ESP_028592_1940   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.01

321.

-16.

6.131

50.1

52.1

Extensive Outcrops of Rhythmic Stratigraphy in Arabia Terra:   ESP_027918_1905   ESP_027984_1905   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.30

1.23

3.76

-15.5

49.8

51.5


  


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