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.

Patchy South Polar Residual Cap in Summertime:   ESP_023807_0885   ESP_023713_0915   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.6

46.0

20.6

16.86

87.1

84.8

Recurring Slope Linea Formation in a Well-Preserved Crater:   ESP_023586_1425   ESP_024008_1425   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.0

192.

-3.1

-14.6

42.7

50.0

Possible Landing Site in Mounds in Central Chryse Region:   ESP_023739_2065   ESP_024016_2065   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
26.28

326.

2.40

-20.8

43.6

42.9

Tilted Layered Feature among Mesas in Southwest Utopia Planitia:   ESP_023603_2175   ESP_024315_2175   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.34

77.9

0

19.54

52.9

43.8

Basal Exposure of South Polar Layered Deposits:   ESP_023773_1025   ESP_023615_1025   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-77.2

129.

25.3

8.468

75.0

73.1

Dark Lanes in South Polar Residual Cap:   ESP_023543_0905   ESP_023531_0905   (Interval in Earth days: 0)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-89.2

340.

26.5

25.47

81.3

81.5

Well-Preserved 6-Kilometer Impact Crater:   ESP_023828_1820   ESP_031819_1820   (Interval in Earth days: 622)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.091

59.3

4.49

-6.67

33.0

37.8

Exposure of South Polar Layered Deposits:   ESP_023795_0925   ESP_023691_0925   (Interval in Earth days: 8)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.4

279.

18.1

2.542

84.6

84.6

Possible Hematite and Kieserite in Capri Chasma:   ESP_023753_1660   ESP_024320_1660   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.8

309.

-4.7

8.069

34.3

39.8

Small Floral-Shaped Volcano on a Cerberus Fossa:   ESP_023811_1880   ESP_024378_1880   (Interval in Earth days: 45)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.076

162.

7.71

21.56

34.0

33.7


  


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