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.

Layering in Heavily Cratered Lucus Planum Terrain:   ESP_087820_1755   ESP_088110_1755   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.46

179.

0.91

19.03

56.1

56.1

Inverted Drainage Network Deep in Central Valles Marineris:   ESP_087816_1705   ESP_088027_1705   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.41

289.

6.89

-9.49

58.7

60.7

Light-Toned Fractured Material West of Nectaris Montes:   ESP_087710_1655   ESP_087644_1655   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.4

303.

1.75

21.48

61.6

59.9

Athabasca Valles:   ESP_087834_1895   ESP_088401_1895   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.534

156.

-2.1

-25.3

49.0

52.7

Layered Rock Exposures in North Hellas Planitia:   ESP_087745_1505   ESP_088391_1505   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.2

69.5

8.55

23.00

71.6

73.2

Terrain Sample:   ESP_087959_1825   ESP_088249_1825   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.270

343.

-2.2

14.54

53.2

52.9

Erosional Features in Medusae Fossae Formation:   ESP_087821_1805   ESP_088032_1805   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.672

151.

6.19

-10.5

52.8

54.9

Channels Going Into Echus Chasma:   ESP_087724_1850   ESP_088792_1850   (Interval in Earth days: 84)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.863

278.

5.37

-4.74

50.2

53.9

Kasei Valles Scarps and Terraces:   ESP_087921_2055   ESP_087855_2055   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.07

301.

-29.

-8.33

46.5

44.4

North-Pole-Facing Deposit in Crater:   ESP_087778_2285   ESP_088068_2285   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
48.34

240.

-10.

2.734

44.8

43.5


  


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