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.

Flow Associated with Hrad Vallis:   ESP_035798_2140   ESP_037077_2140   (Interval in Earth days: 100)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.85

140.

5.93

24.47

42.8

50.6

Cerberus Region Intra-Crater Dune Field:   ESP_035929_1885   ESP_036285_1885   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.525

169.

-8.9

11.89

51.4

50.5

Exposure of North Polar Layered Deposits:   ESP_035605_2660   ESP_036013_2660   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
85.87

328.

-0.4

9.648

60.9

62.4

Candidate Landing Site for InSight:   ESP_035785_1840   ESP_036062_1840   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.050

138.

21.9

0.533

51.0

53.0

Candidate Landing Site for 2020 Mission in West Meridiani Planum:   ESP_035975_1795   ESP_036252_1795   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.58

351.

23.9

4.956

53.6

55.1

High-Latitude Dune Footprints:   ESP_035684_2650   ESP_035922_2650   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.93

339.

0.50

-13.5

60.3

62.0

North Polar Layered Deposits Exposure:   ESP_035652_2660   ESP_035943_2660   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
85.90

122.

1.50

-13.9

61.0

62.7

Dark-Capped Plain and Hills in Western Arabia Region Intercrater Terrain:   ESP_035883_1995   ESP_036806_1995   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.50

342.

-1.6

17.24

46.6

48.9

Crater Ejecta in Terra Sirenum:   ESP_035875_1470   ESP_035941_1470   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.8

206.

10.8

-8.45

75.4

76.3

Monitor Dunes in Crater Northeast of Syrtis Major:   ESP_035919_2005   ESP_035774_2005   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.25

79.1

8.77

-9.01

45.6

46.6


  


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