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.

Channel-Like Features in Cerberus Region:   ESP_066589_1935   ESP_075175_1935   (Interval in Earth days: 668)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
13.50

153.

9.00

7.223

53.3

54.5

Southern Arcadia Planitia:   ESP_066574_2185   ESP_066442_2185   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.33

199.

6.65

25.27

71.2

71.5

Relatively Pristine 7-Kilometer Crater with Gullies:   ESP_066597_1435   ESP_066465_1435   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.3

302.

1.02

24.41

39.4

37.9

Ridges and Channels in Memnonia Sulci:   ESP_066522_1690   ESP_066456_1690   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.9

185.

-1.8

12.74

42.2

41.8

Crater Fill in Noachis Terra:   ESP_066594_1385   ESP_075668_1385   (Interval in Earth days: 707)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.2

25.4

-5.2

-18.0

41.0

40.4

Subtle Topography on South Polar Layered Deposits:   ESP_066773_0905   ESP_066893_0905   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-89.3

215.

28.8

26.44

68.6

70.4

Outflow Channel Floor in Hydraotes Chaos:   ESP_066530_1785   ESP_066596_1785   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.53

325.

7.01

-7.19

45.5

45.8

Sinuous Ridge and Channels in Young Mantle Deposits:   ESP_066617_1400   ESP_066749_1400   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.5

117.

-4.5

-25.0

40.5

42.2

Possible Volcanic Vent East of Olympus Mons:   ESP_066784_1955   ESP_067470_1955   (Interval in Earth days: 53)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.35

232.

4.57

21.83

52.5

44.4

Oyama Crater:   ESP_066780_2040   ESP_066991_2040   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.79

340.

-1.6

21.25

58.6

54.7


  


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