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.

Landforms above Subsurface Radar Observations of South Polar Cap:   ESP_084340_0950   ESP_084301_0950   (Interval in Earth days: 3)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-84.8

177.

8.92

-6.44

65.6

66.5

Fresh 500-meter Diameter Impact Crater:   ESP_084408_1745   ESP_085199_1745   (Interval in Earth days: 62)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.54

93.1

-3.5

19.38

39.7

33.7

Layering in Meridiani Planum Crater:   ESP_084161_1810   ESP_084517_1810   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.786

356.

2.30

-7.87

45.2

41.8

South Facing Gullies with Inverted Aprons:   ESP_084300_1410   ESP_084234_1410   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.8

166.

-3.6

19.20

38.3

36.7

Well-Preserved Impact Crater:   ESP_084209_1585   ESP_084644_1585   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.0

128.

4.91

22.15

36.6

32.9

Inverted Channel in Noachis Terra:   ESP_084385_1585   ESP_084451_1585   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.1

2.82

0.76

-22.6

35.6

37.2

Fluvially Incised Terrain Northeast of Syrtis Major Planum:   ESP_084369_2100   ESP_084514_2100   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
29.56

73.9

-5.8

4.318

62.3

59.8

Potential Fan Deposit in Crater near Mawrth Vallis:   ESP_084425_1990   ESP_084491_1990   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.82

343.

19.4

-2.18

52.3

52.7

Landforms above Subsurface Radar Observations of South Polar Cap:   ESP_084261_0935   ESP_084247_0935   (Interval in Earth days: 1)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-86.5

200.

0.09

14.22

67.1

65.7

Possible Volcanic Edifice in Terra Sirenum:   ESP_084206_1530   ESP_084562_1530   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.8

211.

2.15

-8.24

36.4

35.9


  


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