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.

Crater Floor:   ESP_037851_1780   ESP_038405_1780   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.92

257.

12.7

-0.09

55.8

56.6

Landforms Northeast of Hellas Region:   ESP_037686_1505   ESP_037963_1505   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.1

85.5

6.26

-10.0

62.9

61.5

Arabia Terra:   ESP_037833_1855   ESP_038387_1855   (Interval in Earth days: 43)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.256

28.2

8.61

-6.09

56.1

58.7

Light-Toned Deposits Exposed along Floor of Terra Sabaea Crater:   ESP_037673_1550   ESP_038240_1550   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.8

80.8

-6.4

23.83

62.4

55.3

InSight Mission Candidate Landing Site:   ESP_037829_1840   ESP_038383_1840   (Interval in Earth days: 43)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.983

137.

10.4

-4.64

55.9

58.2

Channelized Flow in Arimanes Rupes Region East of Mangala Valles:   ESP_037734_1675   ESP_046754_1675   (Interval in Earth days: 703)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.2

213.

1.74

-10.3

58.0

53.1

Crater in Tempe Terra:   ESP_037691_2170   ESP_045999_2170   (Interval in Earth days: 647)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.64

299.

13.0

-7.66

60.2

51.0

Hebes Chasma:   ESP_037705_1790   ESP_046659_1790   (Interval in Earth days: 698)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.05

283.

-2.8

8.6

56.8

50.8

External Ponded and Pitted Materials Off Western Rim of Mojave Crater:   ESP_037888_1875   ESP_063233_1875   (Interval in Earth days: 1975)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.393

326.

8.82

-17.0

56.4

53.8

Channel Intersection with Aram Chaos:   ESP_037782_1825   ESP_038402_1825   (Interval in Earth days: 48)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.655

340.

5.31

-25.6

56.2

59.7


  


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