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.

Light-Toned Layered Bedrock Exposed in Valles Marineris :   PSP_002722_1665   PSP_003355_1665   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.1

295.

2.08

-13.4

56.1

53.6

Light-Toned Layering in Plains South of Melas Chasma :   PSP_002617_1690   PSP_003118_1690   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.0

281.

-0.7

24.63

56.4

52.2

Eroded Layers and Scallops and Polygons:   PSP_001964_2275   PSP_003177_2275   (Interval in Earth days: 95)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
46.94

101.

-0.2

25.63

57.4

73.6

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

Gully Orientation Survey:   PSP_001823_1320   PSP_001691_1320   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-47.4

4.36

-0.8

13.07

78.0

78.5

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

59.2

Central Uplift of an Impact Crater:   PSP_002353_1585   PSP_003408_1585   (Interval in Earth days: 82)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.4

290.

0

-26.3

60.2

53.6

Layered Deposit in a Small Crater within Schiaparelli Crater:   PSP_002363_1800   PSP_002508_1800   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.18

14.4

7.82

23.78

54.7

53.5

Channels South of the Base of Ascraeus Mons:   PSP_001985_1860   PSP_002486_1860   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.998

254.

-3.9

22.18

54.0

53.5

Northern Plains Sample:   PSP_001945_2515   PSP_002077_2515   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
71.07

252.

2.20

-10.6

67.4

70.6


  


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