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.

Gullies:   PSP_007771_2290   PSP_008061_2290   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
48.73

318.

-5.4

3.824

45.5

43.7

Mounds in Cydonia Region:   PSP_007770_2205   PSP_007981_2205   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.03

345.

7.20

-6.26

41.7

42.5

Faulted Layered Deposits in Eastern Candor Chasma:   PSP_007192_1710   PSP_008049_1710   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.72

295.

7.77

-11.1

45.4

55.7

Interior Channel in Durius Valles:   PSP_007012_1630   PSP_007157_1630   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-16.8

171.

-3.9

8.48

48.0

49.2

Light-Toned Outcrops in North Melas Chasma Wall with Possible Sulfates:   PSP_007390_1700   PSP_007680_1700   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.78

289.

-8.0

6.442

49.4

51.7

Lobate Debris Aprons with Ridge-Like Structures:   PSP_007693_2300   PSP_008550_2300   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
49.57

286.

6.42

-7.47

45.2

44.0

Light Outcrop in Aurorae Chaos:   PSP_007705_1730   PSP_009498_1730   (Interval in Earth days: 140)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.78

327.

-5.9

5.161

51.2

59.1

Landslide Scarp:   PSP_007785_1645   PSP_008141_1645   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.1

303.

7.47

-3.79

56.0

60.0

Streamlined Form North of Mangala Valles:   PSP_007683_1805   PSP_009542_1805   (Interval in Earth days: 145)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.500

207.

-3.0

-16.3

47.1

56.6

Flow Feature on Eos Chasma Wall:   PSP_007389_1665   ESP_026324_1665   (Interval in Earth days: 1475)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.4

317.

-2.5

19.41

51.1

59.2


  


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