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.

Floor of Mawrth Vallis:   ESP_014007_2030   ESP_022578_2030   (Interval in Earth days: 668)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.98

341.

9.10

25.33

53.5

54.6

Possible Rootless Cones in Hydraotes Chaos:   ESP_013177_1800   ESP_021458_1800   (Interval in Earth days: 645)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.053

326.

-4.9

-21.2

49.8

53.9

Central Structure of a Large Impact Crater:   ESP_013134_1610   ESP_021494_1610   (Interval in Earth days: 652)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.6

62.6

-6.3

14.94

43.1

44.9

Fretted Terrain-Like Aprons Near Reull Vallis:   ESP_013001_1415   ESP_013146_1415   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.4

97.3

-15.

-1.78

44.3

41.5

Valleys and Layering along Melas Chasma:   ESP_013561_1705   ESP_013983_1705   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.60

283.

-0.8

-18.8

40.4

37.5

Olympus Mons Aureole:   ESP_013273_2015   ESP_014262_2015   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.19

220.

12.1

-1.21

60.9

49.4

East Slope of Asimov Crater Central Pit:   ESP_013189_1330   ESP_013835_1330   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.8

5.12

-5.7

20.37

43.1

39.0

Pit with Layered Walls in Mid-Latitude Mantling Unit:   ESP_013951_1225   ESP_021731_1225   (Interval in Earth days: 606)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-57.3

82.3

2.27

-20.0

47.0

49.7

Putative Paleolake:   ESP_013780_1630   ESP_058667_1630   (Interval in Earth days: 3497)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-16.7

64.7

1.57

-15.2

35.8

31.8

Unnamed Central Pit Crater in Daedalia Planum:   ESP_012878_1480   ESP_013155_1480   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.7

212.

4.69

-20.0

43.9

42.3


  


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