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.

Possible Eroded Dyke System in Atlantis Chaos:   ESP_092593_1450   ESP_092224_1450   (Interval in Earth days: 29)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.7

183.

17.5

-7.74

38.6

45.1

Rock Glacier-Like Features:   ESP_092481_1390   ESP_092257_1390   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.4

3.96

7.89

-11.8

41.4

45.6

Possible Channel Linked to Lobate Debris Apron:   ESP_092306_1390   ESP_092227_1390   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.8

102.

19.5

-5.98

42.6

45.6

Dune Field:   ESP_092590_1725   ESP_092946_1725   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.35

263.

-4.9

-19.7

45.7

42.6

Ice Margin of Lobate Debris Apron:   ESP_092504_1370   ESP_092715_1370   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-42.8

97.1

-1.2

-21.8

42.3

42.1

Rock Glacier-Like Feature:   ESP_092547_1380   ESP_092758_1380   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.5

1.56

8.51

-12.4

40.9

40.6

South Polar Layered Deposits:   ESP_092498_0910   ESP_092459_0910   (Interval in Earth days: 3)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.7

296.

25.5

22.97

64.6

64.9

Hillslope Morphologies near Eberswalde Crater:   ESP_092601_1550   ESP_092812_1550   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.7

325.

-4.5

-25.4

40.5

39.9

Streamlined Shapes South of Harmakhis Vallis:   ESP_092425_1385   ESP_092636_1385   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.0

93.9

2.97

-20.3

42.5

42.2

Dune Survey:   ESP_091957_1320   ESP_092313_1320   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-47.4

273.

-8.5

4.482

51.0

45.2


  


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