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_076606_2230   ESP_077292_2230   (Interval in Earth days: 53)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.89

326.

-0.9

-13.6

57.6

51.0

Small Delta or Fan:   ESP_076604_2150   ESP_077290_2150   (Interval in Earth days: 53)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.90

21.3

4.73

-10.0

51.7

46.6

Youthful Crater in THEMIS V22898007 and at Edge of MOC E11-03928:   ESP_076415_1345   ESP_084037_1345   (Interval in Earth days: 594)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-45.2

150.

5.97

-6.29

48.5

41.2

Lobate Feature in Post-Glacial Region:   ESP_076568_2065   ESP_076700_2065   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
26.44

284.

5.84

-21.8

46.6

47.3

Southernmost Extent of South Polar Residual Cap:   ESP_076493_0900   ESP_076151_0900   (Interval in Earth days: 26)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-89.7

249.

29.8

29.68

82.3

76.8

Contact between Wallrock and Interior Layered Deposits in Melas Chasma:   ESP_076634_1660   ESP_077676_1660   (Interval in Earth days: 81)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.6

289.

-9.2

5.336

37.7

49.1

Aeolian Erosion of Medusa Fossae Formation:   ESP_076386_1760   ESP_076241_1760   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.93

214.

25.0

0.959

33.5

35.6

Small Candidate Lake Deposit Downstream of Alluvial Fan:   ESP_076629_1675   ESP_076972_1675   (Interval in Earth days: 26)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.5

66.0

-6.2

-19.7

37.3

41.7

Streamlined Hills in Osuga Valles:   ESP_076435_1640   ESP_076369_1640   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-16.0

320.

5.27

22.25

35.6

33.7

Crater in Crater Exposing Bedrock:   ESP_076436_1560   ESP_076858_1560   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.5

294.

-2.3

24.42

38.2

41.4


  


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