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.

Ridge in Utopia Planitia :   ESP_046824_2155   ESP_046969_2155   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.00

96.2

-7.5

3.307

61.6

62.7

Ice-Rich Deposits in Ancient Valleys :   ESP_046716_1415   ESP_064742_1415   (Interval in Earth days: 1405)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.2

172.

6.21

-3.51

60.1

60.2

Possible Skylight Near Elysium Region :   ESP_046730_2110   ESP_055169_2110   (Interval in Earth days: 658)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
30.56

141.

9.87

-13.7

57.2

55.4

Candidate Recent Impact Site :   ESP_046707_2220   ESP_055146_2220   (Interval in Earth days: 658)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.45

48.7

-1.4

-21.1

62.4

59.2

Candidate ExoMars Landing Site in Oxia Palus :   ESP_046934_1990   ESP_064182_1990   (Interval in Earth days: 1344)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.66

335.

-5.7

-17.8

56.4

59.2

Northern Ejecta and Rays of Istok Crater :   ESP_046686_1350   ESP_064580_1350   (Interval in Earth days: 1394)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-44.8

274.

-5.2

19.11

64.4

62.9

Possible Gullies :   ESP_046883_2105   ESP_064632_2110   (Interval in Earth days: 1383)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
30.20

285.

-3.5

6.966

59.9

65.0

Youthful Dark Rayed Crater with Boulders in Primary Ejecta Deposit :   ESP_046618_1770   ESP_047330_1770   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.07

324.

-8.1

2.309

52.2

51.0

Monitor Seasonal Changes at South Polar Cracked and Gullied Site :   ESP_046892_0980   ESP_046945_0980   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-81.6

66.2

4.68

-8.76

81.2

81.2

Monitoring Region Dubbed Ithaca :   ESP_046770_0950   ESP_046769_0950   (Interval in Earth days: 0)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-85.1

180.

-6.4

20.15

86.7

84.5


  


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