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.

Light-Toned Layering in Noctis Labyrinthus Pit:   ESP_016898_1695   ESP_019377_1695   (Interval in Earth days: 193)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.4

261.

-4.2

-21.4

56.2

59.9

Northern Plains West of Erebus Montes:   ESP_016782_2205   ESP_028531_2205   (Interval in Earth days: 915)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.06

182.

-7.6

11.26

42.3

55.0

Well-Preserved Crater in Margaritifer Terra:   ESP_016407_1675   ESP_016763_1675   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.5

345.

-0.5

12.61

52.5

55.3

Central Uplift and Olivine-Rich Ponded Material in Elorza Crater:   ESP_016659_1710   ESP_017081_1710   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.77

304.

10.5

-3.93

52.2

56.4

Crater in Acidalia Planitia:   ESP_016841_2340   ESP_017830_2340   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
53.72

7.48

5.69

-6.67

45.4

44.9

Terrain South of Newcomb Crater:   ESP_016736_1520   ESP_068970_1525   (Interval in Earth days: 4070)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.6

5.59

4.65

-7.50

65.7

63.9

Debris Apron Source Area:   ESP_016673_2255   ESP_017741_2255   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
45.29

276.

-1.2

10.92

43.4

41.3

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

Submerged Rim of Crater and Floor Deposits from Uzboi Vallis:   ESP_016487_1495   ESP_017120_1495   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-30.0

323.

11.7

-6.42

64.1

71.3

Rocky Mesas in Western Elysium Planitia:   ESP_016889_1885   ESP_017311_1885   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.145

143.

7.82

-11.8

45.3

48.9


  


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