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.

Inverted Channel in Noachis Terra:   ESP_092678_1610   ESP_092177_1610   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.9

22.8

-12.

8.654

41.2

45.8

Crater-Related Pitted Materials in 3-Kilometer Crater in Nepenthes Planitia:   ESP_092411_1960   ESP_092622_1960   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.73

108.

5.50

-22.3

59.7

59.6

Alluvial Fan in Kasei Vallis:   ESP_092602_2030   ESP_092681_2030   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.70

292.

-2.3

24.40

63.3

61.0

North Slope Climbing Dunes in Central Coprates Chasma:   ESP_092602_1665   ESP_092233_1665   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.2

296.

3.95

-23.1

42.6

49.0

Banded or Layered Megabreccia Clasts in Nili Fossae:   ESP_092544_1995   ESP_092610_1995   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.17

76.5

-1.1

-26.7

61.3

62.3

Light Tone Exposures on Floor of Coprates Chasma:   ESP_092628_1645   ESP_092259_1645   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.1

305.

12.1

-12.6

41.1

47.4

Dune Field:   ESP_092506_1945   ESP_093007_1945   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.45

34.8

0.29

-9.08

58.4

53.5

Landforms above Subsurface Radar Observations of South Polar Cap:   ESP_092561_0990   ESP_084729_0990   (Interval in Earth days: 610)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-81.0

352.

10.6

-5.34

60.0

68.1

Crater with Ice Deposit Plus Rim Erosion and Gullies:   ESP_092582_1425   ESP_092938_1425   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.9

126.

-2.7

-15.6

40.6

38.8

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


  


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