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.

Crater Fill Material:   ESP_066791_2045   ESP_067411_2045   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.10

40.8

-4.5

19.86

58.8

50.1

Subtle Scarp in South Polar Layered Deposits:   ESP_066852_0920   ESP_067078_0920   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.8

221.

18.9

8.195

69.2

73.9

Slope Streaks in Arabia Terra:   ESP_066514_2050   ESP_074889_2050   (Interval in Earth days: 652)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.59

40.0

-5.9

9.124

62.5

64.9

Gully Topography:   ESP_066877_1410   ESP_067154_1410   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.8

221.

0.56

15.26

40.3

41.1

Lava Flow in Kasei Valles:   ESP_066848_1985   ESP_067323_1985   (Interval in Earth days: 37)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.53

285.

-2.5

-15.5

54.3

50.0

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

Elaver Vallis:   ESP_066623_1700   ESP_074220_1700   (Interval in Earth days: 592)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.78

309.

-5.2

22.35

42.0

50.7

Clay-Rich Stratigraphy South of Coprates Chasma:   ESP_066531_1650   ESP_067626_1650   (Interval in Earth days: 85)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.9

301.

-8.7

5.387

41.4

39.1

Measure Interaction between Wrinkle Ridge and Paleodune Strata:   ESP_066818_1865   ESP_073993_1865   (Interval in Earth days: 559)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.579

25.5

4.36

22.54

46.9

57.3

Layered Deposits within Depression in Osuga Valles:   ESP_066583_1650   ESP_065897_1650   (Interval in Earth days: 53)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.8

322.

-10.

10.02

41.2

46.6


  


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