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.

Ridges in Nilosyrtis Mensae:   ESP_088312_2135   ESP_088246_2135   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.36

60.4

2.84

21.93

43.1

41.2

Dune Monitoring in Northern Mid-Latitude Crater:   ESP_088259_2385   ESP_088391_2385   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
58.07

62.2

6.70

-16.8

45.9

48.1

Dunes in Crater:   ESP_088355_2370   ESP_088368_2370   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
56.69

322.

0.37

27.25

46.2

43.8

Distinct Crater Wall Layers in Oxia Planum:   ESP_088236_1995   ESP_087946_1995   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.08

338.

-1.7

-16.6

46.5

47.0

Sedimentary Deposits in Chryse Planitia:   ESP_088092_2050   ESP_088527_2050   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.88

309.

-6.8

17.17

44.9

43.9

Jezero Crater:   ESP_088061_1985   ESP_088272_1985   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.47

77.3

-10.

-24.7

46.9

48.7

Athabasca Valles:   ESP_088177_1855   ESP_088467_1855   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.328

151.

-4.9

13.93

52.5

51.8

Terrain in Crater in Tempe Terra:   ESP_088260_2150   ESP_088827_2150   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.74

40.1

2.83

-11.4

42.9

45.9

Dune Field:   ESP_088070_2535   ESP_088413_2535   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
73.41

178.

0.65

-15.8

53.4

54.6

North-Pole-Facing Deposit in Crater Associated with Headwall Erosion:   ESP_088186_2175   ESP_088753_2175   (Interval in Earth days: 45)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.39

260.

0.31

-14.6

42.8

45.7


  


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