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.

Layered Mesa near Mawrth Vallis:   ESP_076553_2040   ESP_076698_2040   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.62

336.

-8.0

17.59

46.1

43.0

Landslide Facing East near Aeolis Mensae:   ESP_076613_1735   ESP_077655_1735   (Interval in Earth days: 81)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.41

141.

4.28

21.20

35.6

44.2

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

Sedimentary Fan in Crater in Terra Cimmeria:   ESP_076652_1445   ESP_077140_1445   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.9

161.

-3.9

15.93

46.4

53.0

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

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

Fluvial Erosion in Phlegra Montes:   ESP_076480_2195   ESP_076823_2195   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.32

164.

8.29

-4.69

56.2

52.8

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

Small Delta or Fan:   ESP_076526_2030   ESP_077212_2030   (Interval in Earth days: 53)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.52

351.

9.17

-11.8

44.5

42.2

Crater on South Polar Layered Deposits:   ESP_076642_0915   ESP_059010_0915   (Interval in Earth days: 1374)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.4

88.0

29.7

26.31

83.7

83.9


  


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