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.

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

Fault Relays in the Cerberus Fossae:   PSP_007645_1885   PSP_007856_1885   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.465

164.

-5.5

-23.3

43.9

46.8

Floor and Central Uplift of Mazamba Crater in Thaumasia Planum:   PSP_007100_1520   ESP_033248_1520   (Interval in Earth days: 2038)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.5

290.

-1.6

-23.6

55.6

51.8

Middle Section of Northern Olympus Mons Basal Scarp:   PSP_007089_2035   PSP_007946_2035   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.25

223.

7.43

-6.64

38.8

42.1

Region Showing Differentially-Eroded Distal Fan Deposits:   PSP_007688_1575   PSP_008545_1575   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.0

72.9

6.99

-15.6

59.4

68.1

Light-Toned Layered Deposits Along Plains South of Ius Chasma:   PSP_007786_1710   PSP_009935_1710   (Interval in Earth days: 167)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.74

276.

-4.8

20.55

52.9

58.8

Thinly-Banded Light-Toned Rock in Unnamed North Sinus Meridiani Crater:   PSP_007084_1845   PSP_007440_1845   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.433

2.80

3.48

-6.89

39.8

43.7

Fan in Aeolis Region:   PSP_007975_1755   PSP_009623_1755   (Interval in Earth days: 129)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.65

154.

-4.9

5.617

52.4

57.8

Area Near Summit of Gale Crater Mound:   PSP_008002_1750   PSP_009927_1750   (Interval in Earth days: 151)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.85

137.

-5.8

-22.8

52.8

59.9

Lineated Valley Fill in Deuteronilus Mensae:   PSP_007795_2175   PSP_009588_2175   (Interval in Earth days: 140)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.35

24.6

-4.2

7.505

42.0

44.3


  


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