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.

Outcrop in Athabasca Valles Lava:   ESP_082705_1880   ESP_082270_1880   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.779

149.

27.6

7.677

57.8

59.0

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

Small Sinuous Ridge at Base of Small Hill in Aeolis Dorsa:   ESP_082560_1735   ESP_082771_1735   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.46

153.

0.76

-24.1

56.7

57.7

Complex Crater near Streamlined Feature in Bahram Vallis:   ESP_082673_1970   ESP_082963_1970   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.79

304.

7.69

19.83

63.0

62.5

Layered Deposits in Burroughs Crater:   ESP_082720_1075   ESP_082878_1075   (Interval in Earth days: 13)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-72.4

117.

0.60

21.39

67.4

63.2

Ridges and Fractures in Sublimation-Pit Crater with Hale Crater Ejecta:   ESP_082620_1415   ESP_082844_1415   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.0

319.

-7.3

22.81

57.5

51.8

Ancient Crust Outcrops in Coprates Chasma:   ESP_082515_1650   ESP_082594_1650   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.9

304.

-14.

15.33

57.4

54.4

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

Layered Deposits in Liais Crater:   ESP_082694_1045   ESP_082681_1045   (Interval in Earth days: 1)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-75.4

106.

8.06

-8.39

68.8

70.2

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


  


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