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.

Baldet Crater Dune Changes:   ESP_080229_2030   ESP_080295_2030   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.68

65.8

1.70

-15.0

48.5

50.2

Aram Chaos:   ESP_080285_1830   ESP_080351_1830   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.757

338.

16.3

-2.05

54.8

56.3

Ice-Rich Deposits in Arabia Terra:   ESP_080204_2145   ESP_080138_2145   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.14

27.7

-8.5

6.219

47.6

46.0

Athabasca Valles:   ESP_080450_1890   ESP_080951_1890   (Interval in Earth days: 40)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.124

155.

-7.0

8.08

54.1

54.1

Dune Interaction with Residual Polar Ice:   ESP_080372_2605   ESP_080280_2605   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.58

98.0

7.78

-6.43

60.8

61.0

Light-Toned Exposures near Voeykov Crater:   ESP_080340_1465   ESP_080274_1465   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.0

283.

-1.3

15.81

77.0

76.2

Possible Dipping Layers in Ice-Affected Crater:   ESP_080515_2115   ESP_080805_2115   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
31.38

178.

-3.2

15.42

49.2

49.7

Floor of East Coprates Chasma:   ESP_080471_1650   ESP_080972_1650   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.0

304.

7.33

20.06

64.8

62.3

Dune Monitoring in Northern Mid-Latitude Crater:   ESP_080576_2395   ESP_080286_2395   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
59.33

302.

24.5

7.497

51.7

50.5

Terrain Sample in Cydonia Region:   ESP_080535_2210   ESP_080970_2210   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.76

350.

0

24.49

49.3

51.2


  


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