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 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

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

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

Gale Crater:   PSP_001554_1745   ESP_018999_1745   (Interval in Earth days: 1359)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.33

138.

-13.

10.53

57.8

56.0

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

Proposed MSL Site in Meridiani Crater:   PSP_002179_1855   ESP_063535_1855   (Interval in Earth days: 4781)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.421

358.

-3.6

18.24

54.7

52.5

Layers in Eberswalde Crater:   PSP_004000_1560   ESP_012610_1560   (Interval in Earth days: 671)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.8

326.

-1.5

22.31

44.5

46.5

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

Crater in Layered Deposits of West Candor Region :   PSP_002841_1740   PSP_003896_1740   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.75

283.

25.5

-0.71

53.3

50.3

Lots of Layering in Becquerel Crater:   PSP_003656_2015   PSP_005845_2015   (Interval in Earth days: 170)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.31

352.

2.46

-21.8

64.2

45.8


  


Page 840 of 878 (8,772 images)