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.

Sharp-Looking Gullies :   PSP_002888_1400   PSP_004167_1400   (Interval in Earth days: 100)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.6

87.9

-8.1

14.24

61.4

41.4

Pit Crater Chains and Cross-Cutting Graben in Tractus Catena:   PSP_002064_2025   PSP_002776_2025   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.18

255.

-6.8

9.417

53.9

59.1

Gullies Possibly Produced by Snow/Ice Melting :   PSP_003096_1375   PSP_003940_1375   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-42.2

169.

-6.1

-22.4

59.0

47.6

Light-Toned Dome on Northern Plains:   PSP_002233_2225   PSP_002866_2225   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.13

319.

-5.7

-19.4

60.0

70.3

Chasma Boreale Scarp with Possible Gypsum:   PSP_001374_2650   PSP_001518_2650   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
85.02

338.

-7.1

13.56

67.8

68.9

Lineated Valley Fill in Coloe Fossae :   PSP_002902_2205   PSP_003245_2205   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.17

53.8

3.42

-28.6

68.0

74.6

Lobate Debris Apron with Ridge-Like Structures; Tempe Terra/Mareotis Fossae:   PSP_002590_2320   PSP_003078_2320   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
51.77

289.

7.55

-12.9

68.4

77.6

Fractured Mounds at the Southern Edge of Elysium Planitia :   PSP_002542_1765   PSP_003597_1765   (Interval in Earth days: 82)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.25

167.

8.70

-21.0

55.0

54.9

Crater and Extensive Field of Secondary Craters Seen in MOC Image R15-02146:   PSP_002230_1850   ESP_027890_1850   (Interval in Earth days: 1999)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.727

46.1

-7.8

4.118

55.2

51.4

Dark-Toned Unit Exposed atop Crater Ejecta in Meridiani Planum :   PSP_002680_1825   PSP_003392_1825   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.240

-0.3

7.78

29.45

55.2

53.5


  


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