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.

Hydrated Sulfates in Melas Chasma:   ESP_082700_1670   ESP_082990_1670   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.7

290.

3.19

17.88

54.8

51.2

Clusters of Craters and Landform near Hephaestus Fossae:   ESP_082271_2050   ESP_090591_2050   (Interval in Earth days: 649)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.76

121.

-6.6

7.281

64.8

58.1

Channels North of Savich Crater:   ESP_082404_1545   ESP_082984_1545   (Interval in Earth days: 45)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.1

95.8

5.32

20.05

57.3

49.4

Lava-Coated Crater near Kasei Valles:   ESP_082265_1960   ESP_082555_1960   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.66

285.

1.99

21.45

61.3

61.1

Terrain Sample:   ESP_082131_1830   ESP_082408_1830   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.782

343.

9.02

-2.09

57.9

59.0

Erosional Features in Crater in Medusae Fossae Formation:   ESP_082110_1720   ESP_081978_1720   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.82

199.

-12.

23.31

59.3

56.7

Fault Cutting Concentric Crater Fill:   ESP_082133_1470   ESP_082199_1470   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.6

294.

4.03

-11.5

61.8

62.2

Ridges West of Vernal Crater:   ESP_082157_1855   ESP_082368_1855   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.604

353.

7.78

21.08

58.4

57.7

Banded Terrain and Layering in Hellas Planitia:   ESP_082221_1400   ESP_082366_1400   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.9

53.0

6.65

29.05

62.6

58.7

Hillslope Morphologies near Du Martheray Crater:   ESP_082338_1865   ESP_082694_1865   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.348

93.9

4.27

-17.3

59.1

61.0


  


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