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.

Fresh Shallow Valleys in Electris Region:   ESP_032580_1350   ESP_032725_1350   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-44.5

169.

-3.5

8.663

50.8

52.6

Streamlined Forms in Athabasca Valles:   ESP_032699_1875   ESP_033200_1875   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.582

153.

-6.5

8.57

35.5

35.7

Possible Hydrated Silicates in Acidalia Planitia:   ESP_032850_2200   ESP_033641_2200   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.91

347.

-6.6

21.87

50.4

41.9

Streamlined Landforms in THEMIS Image V27359007:   ESP_032745_1415   ESP_032811_1415   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.3

341.

19.2

0.849

47.9

50.1

Layered Materials on Northeast Hellas Region Rim:   ESP_032636_1525   ESP_032781_1525   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.3

78.1

-7.4

7.913

41.3

42.4

Gullied Crater:   ESP_032883_1400   ESP_033173_1400   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.6

175.

-2.3

16.04

52.4

56.3

Viscous Flow:   ESP_032875_2195   ESP_033165_2195   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.34

24.7

-7.0

8.757

49.7

45.9

Thermokarst:   ESP_032872_1405   ESP_040837_1405   (Interval in Earth days: 621)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.2

116.

-3.2

-16.8

52.1

41.5

Very Well-Preserved Crater in Ares Vallis:   ESP_032521_1955   ESP_032943_1955   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.35

331.

8.89

-7.24

37.8

37.5

Light-Toned Stratified Materials in Melas Chasma:   ESP_032747_1690   ESP_033169_1690   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.5

285.

-2.6

-24.4

35.6

42.1


  


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