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.

Landslide Facing West near Cydonia Mensae:   ESP_080456_2115   ESP_080522_2115   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
31.37

347.

12.1

-5.83

47.5

49.5

Curvilinear Ridges on Floor of Shalbatana Vallis:   ESP_080589_1885   ESP_080233_1885   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.367

318.

19.4

-1.16

52.6

53.6

Juventae Chasma Interior Deposit Layers:   ESP_080458_1755   ESP_080669_1755   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.62

297.

11.5

-0.14

58.9

59.5

Grooves and Cataracts in Eos Chasma:   ESP_080576_1665   ESP_080431_1665   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.3

318.

-0.6

-16.6

64.1

65.6

Dunes near Syrtis Major Planum Crater Ejecta:   ESP_080242_1970   ESP_080308_1970   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.58

72.6

-8.3

-24.6

51.1

52.7

Streamlined Features in Athabasca Valles:   ESP_080595_1890   ESP_080740_1890   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.663

156.

6.28

17.47

53.5

52.9

Eroded Sedimentary Rock Layers:   ESP_080568_1670   ESP_080779_1670   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.7

176.

-1.1

-14.0

63.8

64.2

A Fissure Vent East of Olympus Mons:   ESP_080579_1955   ESP_080790_1955   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.48

232.

5.92

-6.42

51.4

53.1

Crustal Blocks in the Walls of Coprates Chasma:   ESP_080616_1640   ESP_078282_1640   (Interval in Earth days: 181)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.6

304.

22.8

-1.64

63.6

58.0

Defrosting Dunes in Chasma Boreale:   ESP_080112_2645   ESP_080139_2645   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.55

336.

8.30

-5.70

61.4

62.2


  


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