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.

Impact Crater on East Side of Gale Crater:   ESP_026502_1750   ESP_026647_1750   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.06

138.

-3.6

13.91

55.8

55.0

Bedrock Stratigraphy Exposed in Crater Wall:   ESP_026333_2015   ESP_026478_2015   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.35

68.7

0.94

15.99

42.4

41.5

Exposed Bedrock in Crater Central Uplift off Thaumasia Planum:   ESP_026496_1610   ESP_027485_1610   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.0

304.

-6.5

5.269

65.1

64.1

Light-Toned Layering along Floor of Small Trough Near Juventae Chasma:   ESP_026272_1730   ESP_026628_1730   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.84

298.

-5.3

6.566

56.2

56.6

Cones and Crater in Isidis Planitia:   ESP_026372_1920   ESP_026438_1920   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.64

83.7

18.6

-2.63

44.7

46.6

Features of Large Lobe Northwest of Pavonis Mons:   ESP_026564_1850   ESP_027553_1850   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.068

244.

-7.0

7.531

50.4

50.7

Dune Motion in Northern Plains Rampart Crater:   ESP_026259_2350   ESP_026549_2350   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
54.64

284.

-5.6

11.61

44.1

42.7

Contacts between Yardang-Forming Material and Platy Flow Material:   ESP_026541_1840   ESP_026607_1840   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.813

152.

5.15

-16.8

50.2

51.9

Pit in Syria Planum:   ESP_026247_1650   ESP_051987_1650   (Interval in Earth days: 2006)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.6

260.

8.36

-6.82

60.4

55.1

Samara Valles and Mars 6 Descent Area:   ESP_026376_1555   ESP_036991_1555   (Interval in Earth days: 827)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.0

340.

-2.2

-20.7

68.0

67.4


  


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