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.

Layers in a Central Mound in Gale Crater:   PSP_001422_1750   PSP_001620_1750   (Interval in Earth days: 15)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.98

137.

2.01

-12.5

56.6

57.6

Best Fan Surfaces in West Holden Crater:   PSP_001468_1535   PSP_002154_1530   (Interval in Earth days: 54)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.5

325.

6.55

-10.2

67.7

64.3

Layered Deposits in Ritchey Crater:   PSP_003249_1510   PSP_003526_1510   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.5

309.

6.98

-18.0

53.0

51.6

Nili Fossae Trough, Candidate MSL Landing Site:   PSP_003086_2015   PSP_003587_2015   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.12

74.2

-6.8

19.81

62.4

62.7

Central Uplift of Ritchey Crater :   PSP_002682_1510   ESP_011635_1510   (Interval in Earth days: 698)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.5

309.

5.53

-13.8

59.3

61.0

Large Area of Light-Toned Layering at Mawrth Vallis:   PSP_001929_2050   PSP_002351_2050   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.96

340.

0

-11.8

52.3

57.4

Putative Polyhydrated Sulfate Deposits in East Melas Chasma:   PSP_003487_1670   ESP_040936_1670   (Interval in Earth days: 2918)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.6

290.

0

-25.0

51.7

35.6

Layered Deposits in Terby Crater:   PSP_001662_1520   PSP_002572_1520   (Interval in Earth days: 71)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.5

74.2

-3.0

-17.3

67.8

61.8

Proposed MSL Site in NE Syrtis Major:   PSP_002809_1965   PSP_006000_1965   (Interval in Earth days: 248)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.45

76.5

0.07

23.03

58.5

38.5

Light-toned Layering on Plains South of the West Candor Region:   PSP_005096_1730   PSP_005241_1730   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.93

283.

-12.

2.319

37.7

35.4


  


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