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.

North-Pole-Facing Deposit in Crater Associated with Headwall Erosion:   ESP_086973_2215   ESP_087685_2215   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.99

257.

-7.4

14.63

44.4

41.4

Groups of Ridges in Granicus Valles:   ESP_087070_2115   ESP_087914_2115   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
31.20

129.

7.14

-2.97

41.2

43.1

Small Mesa:   ESP_087081_2175   ESP_087015_2175   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.39

189.

-8.7

7.839

43.5

42.2

Volcanic Vent Southeast of Pavonis Mons:   ESP_086802_1790   ESP_087079_1790   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.03

249.

8.99

-22.0

45.9

50.7

Layering in Lucus Planum:   ESP_087187_1715   ESP_087464_1715   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.22

177.

29.2

6.933

51.7

55.7

Large Alcove with East-Facing Gullies:   ESP_087010_2370   ESP_087353_2370   (Interval in Earth days: 26)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
56.71

322.

7.32

-16.1

49.4

49.3

Channeled Terraces and Debris Fan in Crater in Arabia Terra:   ESP_087022_2165   ESP_087167_2165   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.93

0.65

-9.7

3.05

43.4

42.1

Hillslope Morphologies near Murray Crater:   ESP_087074_1555   ESP_087219_1555   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.0

28.1

-7.1

10.08

63.0

63.5

Concentric Crater Fill:   ESP_087124_2205   ESP_087190_2205   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.20

93.4

5.73

-9.98

42.7

43.9

Small Shield Volcano East of Ascraeus Mons:   ESP_087118_1920   ESP_087606_1920   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.96

261.

5.03

-20.6

43.8

48.5


  


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