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.

Canyon Walls in Coprates Chasma:   ESP_093129_1660   ESP_093063_1660   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.9

306.

-1.8

21.16

37.1

35.9

Irregular Cellular Structures on Crater Floor East of Icaria Fossae:   ESP_093277_1330   ESP_093343_1330   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.6

230.

3.10

-12.7

41.0

42.4

Alluvial Fan in Melas Chasma:   ESP_093446_1665   ESP_093301_1665   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.4

289.

29.6

16.15

32.3

34.5

Channel Cutting Wrinkle Ridge in Promethei Terra:   ESP_093308_1455   ESP_093163_1455   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.1

102.

-3.7

-19.1

36.6

37.8

Antoniadi Crater Fluvial Features:   ESP_093283_2015   ESP_093863_2015   (Interval in Earth days: 45)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.25

58.0

-0.1

25.38

54.2

45.3

Channels on Bernard Crater Floor:   ESP_093291_1555   ESP_093726_1555   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.0

206.

-10.

11.75

35.5

34.2

Young Outflow in Echus Chasma:   ESP_093354_1805   ESP_093209_1805   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.647

279.

27.9

10.93

38.4

41.3

Arcing Ridge in Meridiani Planum:   ESP_093312_1870   ESP_093246_1870   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.776

347.

11.4

29.84

43.6

43.0

Landforms Above Subsurface Radar Observations of South Polar Cap:   ESP_093425_1015   ESP_084920_1015   (Interval in Earth days: 663)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-78.4

162.

-0.1

17.93

63.9

67.3

Antoniadi Crater Fluvial Features:   ESP_093494_2015   ESP_093217_2015   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.38

58.0

-11.

18.24

52.2

54.0


  


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