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.

Mounds in Chryse Planitia :   ESP_058974_2245   ESP_059475_2245   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.03

313.

-3.7

11.54

56.2

49.1

Well-Exposed Ejecta Blanket at Kontum Crater :   ESP_058896_1480   ESP_058962_1480   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.7

292.

3.30

-18.2

38.8

41.1

Western Half of Well-Preserved Impact Crater :   ESP_058921_2020   ESP_059422_2020   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.61

324.

-6.8

13.21

41.1

36.3

Pitted Cones in Chryse Planitia :   ESP_058723_2160   ESP_059000_2160   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.84

327.

4.89

-20.5

52.8

50.7

Slope Monitoring :   ESP_058715_1500   ESP_059348_1500   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.5

194.

4.51

-20.7

35.1

45.9

Troughs in Acidalia Planitia :   ESP_058987_2245   ESP_058565_2245   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.98

319.

-7.2

8.327

56.1

61.5

Chaos Terrain in Small Impact Crater :   ESP_058965_1495   ESP_059255_1495   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-30.3

210.

-20.

5.926

40.6

43.2

Hunt for Ancient Impact Craters Near Nili Fossae :   ESP_058772_2025   ESP_058706_2025   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.32

72.3

-7.1

14.88

43.0

42.4

Channels in Nilokeras Mensae :   ESP_058816_2100   ESP_076765_2100   (Interval in Earth days: 1398)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
29.61

309.

1.56

-8.48

47.1

47.6

Potential Landing Site in Phlegra Montes :   ESP_058874_2160   ESP_059296_2160   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.84

164.

8.55

-4.42

50.6

46.4


  


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