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.

Canyon Walls in Coprates Chasma:   ESP_087367_1655   ESP_087301_1655   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.2

307.

3.61

24.06

58.9

56.9

Layering within Yardangs:   ESP_087477_1700   ESP_088334_1700   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.71

184.

-2.1

18.83

57.3

60.0

North-Pole-Facing Deposit in Crater Associated with Headwall Erosion:   ESP_087343_2220   ESP_087488_2220   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.44

236.

-6.8

6.862

43.6

42.3

Irregular Cellular Structures around Crater in Arabia Terra:   ESP_087496_2160   ESP_088630_2160   (Interval in Earth days: 88)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.47

20.2

-7.3

-22.0

42.9

46.2

Pitted Cone with Clear Moat:   ESP_086926_2080   ESP_087071_2080   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.85

102.

-8.9

4.814

42.3

41.3

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

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

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

Terrain in Chryse Planitia:   ESP_087129_2145   ESP_087973_2145   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.14

317.

6.55

-6.10

41.6

43.2

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


  


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