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.

Kasei Valles Alluvial Fans:   ESP_088633_2040   ESP_088778_2040   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.55

298

-6.4

3.817

46.5

46.1

North Polar Layered Deposits Structural Geology in Icy Layers:   ESP_088653_2625   ESP_088693_2625   (Interval in Earth days: 3)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
82.34

81.4

8.18

-8.30

58.5

59.6

Crater Exposing Structure of Glacial Fill inside Baphyras Catena:   ESP_088436_2190   ESP_088647_2190   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.53

275.

-8.7

-18.9

44.2

45.8

Channel Entering Sklodowska Crater:   ESP_088512_2130   ESP_088578_2130   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.92

358.

15.6

-3.74

42.6

44.5

Alluvial Fans and Terraced Scarps in Kasei Valles:   ESP_088541_2025   ESP_088330_2025   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.38

291.

-19.

-6.13

47.7

46.0

North Polar Layered Deposits Structural Geology in Icy Layers:   ESP_088733_2630   ESP_088562_2630   (Interval in Earth days: 13)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
82.71

56.5

6.65

-7.41

59.1

59.3

Ridged Flow-Like Features in Deuteronilus Mensae:   ESP_088445_2225   ESP_088511_2225   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.33

26.8

8.67

-8.24

42.8

44.5

Steep Sandy Slopes in Coprates Chasma:   ESP_088554_1660   ESP_088620_1660   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.7

298.

11.2

-14.2

63.4

65.0

Stereo for Kunowsky Crater Dunefield:   ESP_088644_2370   ESP_088420_2370   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
56.72

350.

5.32

-16.7

46.6

47.9

Layering and Contact in Lucus Planum:   ESP_088545_1725   ESP_088756_1725   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.43

184.

-3.0

-16.9

60.3

61.4


  


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