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 Outcrops and Unusual Ridges in Eastern Noctis Labyrinthus:   ESP_015922_1720   ESP_016634_1720   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.04

266.

-0.8

20.76

44.6

50.8

Small Valley in Eastern Hellas Planitia:   ESP_016100_1385   ESP_016166_1385   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.3

91.0

1.60

-16.2

67.7

69.7

Ridge Near Olympus Mons:   ESP_015976_1945   ESP_016899_1945   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.11

229.

-5.1

12.21

39.4

42.7

Stranded Lobe of Material with Associated Ridge on Valley Floor:   ESP_016238_2180   ESP_017161_2180   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.54

273.

-3.4

6.789

42.5

40.5

Lineated Valley Floor Material in Terrain North of Arabia Region:   ESP_016287_2205   ESP_077488_2205   (Interval in Earth days: 4769)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.04

15.5

-2.8

7.652

43.1

46.5

Layered Rocks in Ius Chasma:   ESP_016225_1730   ESP_018348_1730   (Interval in Earth days: 166)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.94

273.

0

-15.1

47.4

59.4

Marte Vallis Streamlined Landforms:   ESP_016202_1895   ESP_016835_1895   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.254

179.

5.93

-8.19

40.6

45.8

Well-Preserved Impact Crater:   ESP_015905_2235   ESP_016182_2235   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.91

3.36

3.72

-15.9

45.9

45.8

Stratigraphic Relations in MOC Image M00-02426 in Sinus Meridiani:   ESP_016169_1790   ESP_019637_1790   (Interval in Earth days: 270)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.77

1.73

4.18

-16.4

43.8

56.0

Gullied Crater Wall:   ESP_015950_1395   ESP_016451_1395   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.3

225.

4.65

25.21

64.5

70.3


  


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