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.

Crater with Lineated Material on Floor:   ESP_016824_1465   ESP_016969_1465   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.2

124.

-2.9

10.86

71.0

71.5

Crossing Wrinkle Ridges and Secondaries in Hesperia Planum:   ESP_016310_1545   ESP_016666_1545   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.2

115.

3.44

15.21

59.1

62.7

Small Crater Exposed in Cross-Section by Erosion:   ESP_016699_1715   ESP_019178_1715   (Interval in Earth days: 193)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.45

293.

1.41

-13.7

52.9

58.8

Olivine-Rich Terrain in Yuty Crater:   ESP_016579_2025   ESP_017647_2025   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.08

325.

1.00

18.99

40.6

42.1

Outcrop of Rhythmic Bedding in Arabia Terra:   ESP_016657_1890   ESP_017013_1890   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.820

358.

-1.3

8.534

44.4

45.7

25-Kilometer Diameter Gullied Impact Crater in Acidalia Planitia:   ESP_016592_2170   ESP_016737_2170   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.54

329.

-3.7

9.38

41.6

40.3

Very Well-Preserved 12-Kilometer Diameter Crater:   ESP_016569_2320   ESP_016846_2320   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
51.40

234.

-1.5

-15.9

46.0

46.1

Possible Phyllosilicate-Rich Area in Syrtis Major:   ESP_016628_2040   ESP_017340_2040   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.69

68.6

-7.2

6.233

41.2

42.0

Fretted Valley Outlet:   ESP_016391_2195   ESP_016668_2195   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.96

56.1

-0.8

-19.4

42.2

43.3

Cerberus Fossae:   ESP_016822_1865   ESP_017600_1865   (Interval in Earth days: 60)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.281

173.

2.06

-11.4

46.2

50.8


  


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