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 MSL Rover Landing and Seismic Network Site in Utopia Region:   ESP_022178_1960   ESP_022534_1960   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.61

105.

-3.8

4.541

55.5

50.9

Stereo of Seasonal/Yearly SPRC Monitoring Site:   ESP_022197_0935   ESP_022592_0935   (Interval in Earth days: 30)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-86.3

3.59

-1.9

8.738

65.0

66.4

Faults in the South Polar Layered Deposits:   ESP_022126_0995   ESP_022100_0995   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-80.2

100.

18.8

-2.52

58.5

59.9

Possible Source Region of Harris Crater Fan:   ESP_022140_1585   ESP_021784_1585   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.4

67.2

3.34

-9.00

37.3

42.6

Possible Future Mars Landing Site with Inverted River Meanders:   ESP_022084_1740   ESP_022361_1740   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.72

153.

12.8

-21.6

42.7

41.8

Polar Cap Seasonal Monitoring Site:   ESP_022170_0945   ESP_022421_0945   (Interval in Earth days: 20)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-85.6

6.48

2.37

-7.73

63.8

65.9

Light and Dark Units Southwest of Eos Chasma:   ESP_022052_1625   ESP_056772_1625   (Interval in Earth days: 2706)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-17.1

309.

0

22.03

39.6

42.5

Polar Ice Monitoring Site:   ESP_022054_0930   ESP_022396_0930   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-86.7

298.

8.73

22.61

64.3

64.2

Inverted Valleys near Juventae Chasma:   PSP_007627_1765   PSP_008563_1765   (Interval in Earth days: 73)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.67

297.

-4.8

5.755

48.7

55.0

Possible Inverted Topography Landscape with Clay Minerals:   ESP_022077_2000   ESP_022367_2000   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.80

342.

-1.5

22.08

59.3

54.9


  


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