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.

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

Dipping Layers in Ejecta:   ESP_076391_2160   ESP_075824_2160   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.65

75.9

-6.4

-18.4

55.5

63.9

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

Troughs and Ridges in Chryse Planitia:   ESP_076659_2105   ESP_077002_2105   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
30.13

321.

2.40

-8.10

48.2

46.0

Stepped Fan on West Crater Wall of Gale Crater:   ESP_076534_1750   ESP_077154_1750   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.00

136.

8.87

-1.44

35.0

40.0

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

Valleys and Inverted Channels in Melas Chasma:   ESP_076621_1710   ESP_076476_1710   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.11

282.

15.2

-14.2

35.0

36.6

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

Exposure of South Polar Layered Deposits within Residual Cap:   ESP_076503_0915   ESP_076225_0915   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.3

308.

22.2

29.52

82.0

76.7

Landslide Scarp and Lobe:   ESP_076597_1540   ESP_076663_1540   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.8

220.

5.92

-9.92

40.3

42.3


  


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