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.

Knobby Unit in Intercrater Plain:   ESP_060819_1575   ESP_060964_1575   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.2

353.

-5.6

15.10

61.0

61.2

Complex Inverted Channels in Aeolis Dorsa:   ESP_060734_1760   ESP_053639_1760   (Interval in Earth days: 552)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.00

153.

-26.

5.933

50.2

53.9

Faulted and Embayed Low Shield East of Pavonis Mons:   ESP_060783_1800   ESP_061139_1800   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.196

253.

-5.6

17.40

46.9

48.0

Layered Structure and Depression on Rim of Moreux Crater:   ESP_060975_2215   ESP_062373_2215   (Interval in Earth days: 109)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.40

46.2

2.98

-29.8

40.0

45.8

Candidate Landing Site for SpaceX Starship East of Arcadia Planitia:   ESP_060811_2205   ESP_060323_2205   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.02

203.

3.50

18.41

39.8

39.8

Eastern Edge of Polar Cap Outlier in Olympia Mensae:   ESP_060340_2540   ESP_060353_2540   (Interval in Earth days: 1)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
73.96

94.3

-7.8

7.097

61.7

60.8

Light-Toned Deposits along Ius Chasma Wallrock:   ESP_060479_1730   ESP_060835_1730   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.15

273.

-9.0

12.07

48.0

50.2

Pitted Cones in Chryse Planitia:   ESP_060490_2170   ESP_060846_2170   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.71

327.

-1.8

13.14

40.0

38.3

Cataract and Grooves in Kasei Valles:   ESP_060320_2030   ESP_059964_2030   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.75

289.

6.80

-8.25

36.9

37.5

Ridged Landforms in Noachis Terra South of Greeley Crater:   ESP_060344_1360   ESP_086363_1360   (Interval in Earth days: 2027)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.5

3.73

-2.7

-12.5

70.6

66.9


  


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