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.

Impact Crater with a Rocky Central Uplift:   ESP_012947_1735   ESP_022441_1735   (Interval in Earth days: 740)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.55

125.

4.88

27.14

48.6

37.0

Stratigraphy of Rocks in Claritas Fossae Region:   ESP_012995_1530   ESP_030902_1530   (Interval in Earth days: 1395)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.9

258.

-7.1

4.769

43.5

37.3

Well-Preserved Impact Crater:   ESP_012851_1270   ESP_013695_1270   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-52.8

234.

-10.

-26.8

49.2

45.2

Wrinkle Ridge in Hesperia Planum:   ESP_013765_1605   ESP_014187_1605   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.3

114.

2.67

-13.1

35.4

34.5

Ganges Mensa Layered Deposits:   ESP_012993_1725   ESP_013059_1725   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.39

310.

-5.5

-26.0

48.5

49.3

Lobate Features in the Charitum Montes:   ESP_013165_1275   ESP_013244_1275   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-51.9

301.

-4.0

20.40

45.0

42.6

Gullies Observed by MOC:   ESP_012707_1445   ESP_013208_1445   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.4

201.

2.07

23.84

46.6

38.4

Sulfate Beds in Gale Crater with Possible Repeating Section:   ESP_012907_1745   ESP_013540_1745   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.32

137.

5.49

-16.2

49.5

43.6

Layering on Floor of Noctis Labyrinthus Pit:   ESP_014076_1680   ESP_021513_1680   (Interval in Earth days: 579)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.8

263.

-5.4

13.21

35.2

46.5

Superb Phyllosilicate Mafic Stratigraphy Northwest of Hellas Planitia:   ESP_012923_1540   ESP_013345_1540   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.9

63.8

-4.0

-17.6

44.3

40.2


  


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