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_084325_1000   ESP_084562_1000   (Interval in Earth days: 19)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-80.0

222.

-6.3

13.65

62.6

64.0

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

Fresh Impact Crater:   ESP_084401_1440   ESP_085324_1440   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.7

287.

3.51

-12.0

36.9

45.2

North Branch of Kasei Valles East of Labeatis Mensa:   ESP_084493_2060   ESP_084058_2060   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.76

287.

8.43

-6.75

57.0

63.3

Recent Crater:   ESP_084414_1385   ESP_084770_1385   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.2

293.

7.28

-8.40

38.5

41.5

Landforms above Subsurface Radar Observations of South Polar Cap:   ESP_084338_0965   ESP_084219_0965   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-83.2

236.

-5.6

8.915

65.3

63.3

Crater in Galaxias Fossae:   ESP_084406_2175   ESP_093016_2175   (Interval in Earth days: 671)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.92

142.

-4.1

23.31

67.4

68.2

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

Gully Monitoring:   ESP_084450_1285   ESP_092335_1285   (Interval in Earth days: 615)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-50.9

33.5

-7.5

4.851

44.2

46.0

Dune Change Detection in Mawrth Vallis:   ESP_084201_1980   ESP_084135_1980   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.79

343.

-5.8

20.45

55.9

55.2


  


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