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.

Valley in Meridiani Planum Highlands and Contact with Plains:   ESP_036186_1760   ESP_036542_1760   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.78

355.

-20.

-2.43

58.6

57.2

Group of Cones with Summit Depressions near Coprates Chasma North Wall:   ESP_036109_1675   ESP_043520_1675   (Interval in Earth days: 577)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.4

297.

0.39

26.06

62.1

55.2

Intracrater Dune Changes:   ESP_036173_1980   ESP_036107_1980   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.97

346.

-5.6

13.20

48.3

46.5

Crater in Central Arabia Terra with Yardangs at Northeast Wall:   ESP_036290_1915   ESP_037358_1915   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.36

33.7

-4.3

14.11

50.7

53.3

Summit Pit Crater in Terra Sirenum:   ESP_036086_1470   ESP_036574_1470   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.9

207.

6.31

-16.4

75.2

74.5

Small Rocky Impact Crater:   ESP_036303_1680   ESP_037160_1680   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.7

42.0

-8.9

14.53

62.0

58.5

Vastitas Borealis Intra-Crater Dunes:   ESP_036344_2520   ESP_036463_2520   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
71.89

344.

8.11

-18.5

56.2

59.4

Monitoring Possible Active Dark Dunes in Arabia Terra:   ESP_036159_1905   ESP_036225_1905   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.60

9.06

5.43

-14.1

49.9

51.6

Topographic Low with Thermally-Distinct Terrain in THEMIS IR Images:   ESP_036135_2185   ESP_036979_2185   (Interval in Earth days: 65)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.54

301.

0.45

-20.5

44.9

54.1

InSight Mission Candidate Landing Site:   ESP_036273_1840   ESP_036207_1840   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.093

137.

5.69

24.35

52.8

51.3


  


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