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.

Possible Fossil Dunes in Noachis Terra:   ESP_032941_1310   ESP_033020_1310   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-48.9

34.0

-2.6

22.11

60.1

60.2

Impact Crater with Central Peak:   ESP_033202_1685   ESP_060393_1685   (Interval in Earth days: 2119)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.5

101.

2.77

-6.13

40.8

49.3

Dark Sediments in the Medusae Fossae Formation:   ESP_032910_1795   ESP_033411_1795   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.53

153.

-6.3

6.617

35.6

38.9

Pedestal Crater in Arcadia Planitia:   ESP_032921_2355   ESP_033145_2355   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
55.13

204.

-0.0

22.74

59.9

55.7

Complex of Fresh Shallow Valleys:   ESP_033134_1385   ESP_068014_1385   (Interval in Earth days: 2718)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.3

162.

-0.6

-21.4

57.7

56.8

Western Portion of Possible Multiple Impact in Arabia Terra:   ESP_033272_1840   ESP_033417_1840   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.045

349.

-3.5

10.60

37.5

37.5

Large Meander in Sinuous Ridge in Aeolis Region:   ESP_033187_1780   ESP_034321_1780   (Interval in Earth days: 88)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.77

150.

-1.5

7.93

37.7

48.4

Possible Preserved Impact Melt Flow on the Ejecta of Bakhuysen Crater:   ESP_033258_1555   ESP_033469_1555   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.1

14.1

6.09

-3.25

47.9

51.7

Possible Terraced Crater in Arcadia Planitia:   ESP_033066_2230   ESP_033501_2230   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.78

209.

-7.0

19.40

50.0

44.4

Massif in Northwest Hellas Region:   ESP_033006_1545   ESP_033296_1545   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.0

55.1

2.01

24.62

44.9

47.9


  


Page 513 of 896 (8,955 images)