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 Unit and Dunes in Coprates Chasma:   ESP_087433_1655   ESP_089002_1655   (Interval in Earth days: 122)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.4

306.

-8.7

10.37

60.3

63.7

Margin of Lobate Deposit in Nereidum Montes:   ESP_087406_1400   ESP_087116_1400   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.7

323.

21.8

-7.50

75.8

74.4

Crater near Cerberus Fossae:   ESP_087280_1890   ESP_087636_1890   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.029

158.

7.69

23.79

45.6

46.3

Ridge in Crater Wall:   ESP_087429_2205   ESP_036342_2205   (Interval in Earth days: 3980)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.13

48.1

-3.5

15.62

43.0

45.0

Planned ExoMars Landing Site in Oxia Planum:   ESP_087234_1990   ESP_087590_1990   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.93

335.

-12.

3.102

44.1

44.2

Small Alluvial Fans in Kasei Valles:   ESP_087156_2065   ESP_087011_2065   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
26.44

299.

26.2

13.41

39.5

40.5

Knob within Kasei Valles Lava:   ESP_087183_2010   ESP_087328_2010   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.53

286.

-6.8

9.822

43.1

42.2

Jarosite-Bearing Terrain in Northern Nili Fossae:   ESP_086927_2070   ESP_088483_2070   (Interval in Earth days: 121)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
26.80

74.9

-6.0

-23.3

42.0

46.9

Hillslope Morphologies near Murray Crater:   ESP_087074_1555   ESP_087219_1555   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.0

28.1

-7.1

10.08

63.0

63.5

Channels in Granicus Valles:   ESP_087017_2080   ESP_087294_2080   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.96

135.

19.2

-2.6

39.9

42.3


  


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