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.

Pitted Mounds in Chryse Planitia:   ESP_063325_2215   ESP_055307_2215   (Interval in Earth days: 624)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.11

331.

-26.

-6.76

53.9

60.3

Chasma Boreale Head Scarp Dunes:   ESP_063323_2650   ESP_063441_2650   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.69

0.77

-8.0

6.363

70.6

71.6

Small Ice-Filled North Polar Layered Deposits Crater:   ESP_063253_2655   ESP_071615_2655   (Interval in Earth days: 651)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
85.65

93.4

0.84

10.75

69.9

64.7

Northern Dunes and Snowfall:   ESP_062901_2560   ESP_054158_2560   (Interval in Earth days: 681)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
75.59

13.4

2.67

-13.6

59.4

60.9

Iani Chaos:   ESP_063206_1780   ESP_063852_1780   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.13

343.

3.24

27.44

55.5

54.1

Layering in Arabia Terra:   ESP_063337_1820   ESP_063403_1820   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.753

6.72

-6.4

-28.7

55.0

57.0

Cratered Cone North of Noctis Fossae:   ESP_063209_1800   ESP_063420_1800   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.10

261.

0.69

-12.9

54.8

56.2

Possible Impact Melt Deposits in a Multiple Impact Structure:   ESP_062296_1840   ESP_062586_1840   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.036

349.

5.58

22.88

51.2

50.4

Dynamic Activity in a Crater North of Antoniadi Crater :   ESP_023261_2065   ESP_023327_2065   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
26.12

57.0

-1.8

-18.8

49.3

49.4

Pollywog Craters on Mars:   ESP_061768_2200   ESP_062045_2200   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.79

0.03

-0.9

-11.2

40.7

42.4


  


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