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.

Mantling Unit in Tithonium Chasma:   ESP_083083_1750   ESP_083149_1750   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.70

271.

4.04

-20.1

53.8

55.1

Channels in Tyrrhena Terra:   ESP_083116_1520   ESP_083327_1520   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.6

93.9

0.05

-5.04

49.2

46.7

Channel with Distinct Levees:   ESP_083006_1575   ESP_083151_1575   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.0

216.

0

12.87

50.9

48.2

Channel Edge with Overbank Flow Deposits:   ESP_083033_1835   ESP_082967_1835   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.456

195.

7.43

29.20

57.0

55.5

Fresh Crater near Ice-Rich Terrain:   ESP_083188_1295   ESP_083254_1295   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-50.3

290.

7.09

-8.45

50.5

50.7

Aeolis Dorsa Deltaic Lobes:   ESP_082995_1735   ESP_083272_1735   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.31

154.

4.37

-26.6

53.9

54.0

Hillslope Morphologies near Holden Crater:   ESP_083002_1550   ESP_083859_1550   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.8

325.

7.31

20.89

50.2

38.3

Noachis Terra Channels:   ESP_083106_1560   ESP_083172_1560   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.9

6.27

2.56

-19.9

49.3

50.2

Eroded Landform in Chryse Planitia:   ESP_083121_1940   ESP_083767_1940   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
13.87

312.

-4.9

22.98

62.5

56.4

Ancient Crust Outcrops at Nectaris Montes:   ESP_082950_1650   ESP_082884_1650   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.7

304.

2.16

26.28

52.4

51.0


  


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