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.

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

Crater Rim Gullies Filled with Small Dunes:   ESP_015934_2165   ESP_037243_2165   (Interval in Earth days: 1660)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.09

292.

1.58

-16.4

42.8

56.6

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

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

Cerberus Fossae Cutting Hill:   ESP_016229_1895   ESP_016862_1895   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.130

162.

4.10

-9.74

40.9

46.1

Possible Phyllosilicate-Rich Terrain:   ESP_016102_2160   ESP_044044_2160   (Interval in Earth days: 2177)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.47

26.3

2.45

19.39

42.0

37.7

Mounds on Hrad Vallis Mudflow:   ESP_016256_2155   ESP_016322_2155   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.06

142.

-2.8

-19.2

41.7

43.0

Juventae Region Mound and Possible Sulfate-Rich Terrain:   ESP_015934_1760   ESP_016646_1760   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.74

298.

0

21.43

42.9

48.4

Crater with Rampart-Like Ejecta Exposed in Cross Section:   ESP_016080_1745   ESP_025574_1745   (Interval in Earth days: 740)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.30

272.

0

11.85

45.1

49.7


  


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