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.

Proposed MSL Landing Site in Holden Crater:   PSP_008193_1535   PSP_008483_1535   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.1

325.

-7.5

0.702

68.1

69.7

Proposed MSL Landing Site in Mawrth Vallis - Ellipse 4:   PSP_008390_2050   PSP_008891_2050   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.79

339.

-7.3

-21.7

43.3

46.0

Small Channel in Elysium Planitia:   PSP_008265_1860   PSP_008990_1860   (Interval in Earth days: 57)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.981

155.

-6.8

12.22

49.1

50.7

Ridges in Huo Hsing Vallis :   PSP_008189_2080   PSP_007833_2080   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.52

67.0

-1.3

7.894

41.8

40.2

Channel into Jezero Crater Delta:   PSP_007925_1990   PSP_008650_1990   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.85

77.5

-7.4

17.24

42.8

43.6

Well Preserved Impact Crater of Alba Patera:   PSP_006745_2250   PSP_007035_2250   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.64

253.

2.65

17.88

49.7

46.1

Catastrophic Flood Channel of Ares Valles:   PSP_007810_1885   PSP_008166_1885   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.543

337.

8.22

-2.42

44.0

47.1

Light-Toned Rocks Exposed inside a Crater:   PSP_008075_1590   PSP_009512_1590   (Interval in Earth days: 112)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.5

306.

-5.2

17.41

63.1

66.9

Segment of a Crater Ray:   PSP_007751_1640   ESP_077325_1640   (Interval in Earth days: 5421)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.9

151.

6.32

-4.44

56.1

46.2

Lava Flows at the Summit of Olympus Mons:   PSP_007959_1980   PSP_009317_1980   (Interval in Earth days: 106)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.75

226.

23.3

3.143

40.8

47.1


  


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