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.

Landforms in Utopia Planitia :   ESP_046521_2125   ESP_046666_2125   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.43

87.2

5.50

18.37

55.5

56.4

Eastern Rim and Ejecta of Resen Crater :   ESP_046415_1520   ESP_046837_1520   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.9

108.

6.36

-3.11

58.8

55.6

Channels in a Crater Northeast of Hellas Planitia:   ESP_046205_1515   ESP_046350_1515   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.4

83.5

-7.4

7.089

61.7

59.5

Lobate Debris Apron in Northwest Argyre Region :   ESP_046566_1335   ESP_046711_1335   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-45.8

309.

-1.9

10.95

66.3

63.4

Lava Flow and Channels near Olympica Fossae:   ESP_046555_2005   ESP_046700_2005   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.43

241.

-8.0

8.018

53.6

53.7

Small Ridges in Rabe Crater :   ESP_046576_1365   ESP_046998_1365   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-42.9

35.4

8.28

-2.65

64.0

58.9

Alluvial Fans in Southwestern Mojave Crater:   ESP_046275_1870   ESP_051958_1870   (Interval in Earth days: 443)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.160

326.

5.60

25.31

49.5

40.4

Light-Toned Material in Fresh Shallow Valleys :   ESP_046458_2160   ESP_050928_2160   (Interval in Earth days: 348)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.49

8.31

-8.2

-25.0

56.9

44.0

Well-Preserved 7-Kilometer Impact Crater :   ESP_046334_2075   ESP_050883_2075   (Interval in Earth days: 355)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.00

154.

-7.3

5.524

52.7

37.9

Transition from Inverted to Depressed Channel in Terra Sirenum :   ESP_046346_1430   ESP_060126_1430   (Interval in Earth days: 1074)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.6

193.

8.10

-1.33

63.5

62.1


  


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