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 Mafic-Rich Armored Ejecta Deposits:   ESP_074190_1195   ESP_074058_1195   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-59.9

61.9

-20.

6.187

58.5

58.6

Small Delta or Fan:   ESP_074002_1760   ESP_074780_1760   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.73

142.

4.88

-22.5

55.2

51.0

Chryse Chaos:   ESP_074114_1860   ESP_073969_1860   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.991

323.

8.91

-5.81

57.9

59.3

Ridges in Huygens Crater:   ESP_074203_1640   ESP_082102_1640   (Interval in Earth days: 615)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.8

56.1

4.52

26.16

50.9

56.9

Light-Toned Outcrops in Aurorae Chaos:   ESP_074259_1725   ESP_082224_1725   (Interval in Earth days: 621)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.36

326.

-4.5

7.8

53.2

57.4

Light-Toned Deposits in Iani Chaos:   ESP_074087_1780   ESP_074021_1780   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.04

342.

-6.0

19.68

56.1

54.4

Channel along Edge of Crater:   ESP_074028_1445   ESP_066233_1445   (Interval in Earth days: 607)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.1

156.

7.22

-5.51

52.2

41.6

Channel Crossing Heavily Eroded Wrinkle Ridge:   ESP_074146_1485   ESP_073790_1485   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.4

175.

-4.9

-20.8

51.1

57.1

Radial Ridges on Crater Floor:   ESP_074151_1520   ESP_074362_1520   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.8

37.1

7.36

-2.80

50.1

48.1

Inlet Valley to Jezero Crater:   ESP_074268_1990   ESP_074413_1990   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.58

76.8

6.94

20.62

63.9

62.7


  


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