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.

Lineated Valley Fill in Coloe Fossae:   PSP_008598_2155   PSP_008954_2155   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.16

57.2

-3.6

-18.8

42.2

44.3

Layers in Uzboi Vallis:   PSP_008338_1525   PSP_010329_1525   (Interval in Earth days: 155)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.4

324.

5.23

-10.4

69.3

70.2

Crater Floor Fan:   PSP_008233_1920   PSP_008879_1920   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.72

307.

6.25

-7.44

45.5

49.1

Hematite in West Candor Chasma:   PSP_007601_1745   PSP_010449_1745   (Interval in Earth days: 222)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.55

286.

7.08

-20.0

48.5

59.7

Bacolor Crater Interior and Central Peak:   PSP_007106_2135   PSP_009677_2135   (Interval in Earth days: 200)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.99

118.

0.49

-21.5

41.8

47.5

Inverted Channel and Fan Draining into Crater:   PSP_008185_1750   ESP_035032_1750   (Interval in Earth days: 2092)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.17

180.

3.94

-14.1

53.7

56.6

Potential Fan Deposit in Ritchey Crater with Clays:   PSP_007363_1510   PSP_008365_1510   (Interval in Earth days: 78)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.4

308.

3.89

-7.30

59.7

71.0

Crater in the Adamas Labyrinthus Region Seen in THEMIS Image V21701005:   PSP_007713_2170   PSP_009862_2170   (Interval in Earth days: 167)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.45

103.

-4.4

10.64

41.9

45.6

Dark Dunes Over Light-Toned Mega-Ripples Seen in MOC Image SP1-26004:   PSP_007532_1905   PSP_008679_1905   (Interval in Earth days: 89)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.61

9.06

2.36

-9.87

41.8

49.2

Central Peak of Fesenkov Crater:   PSP_007931_2020   ESP_024585_2020   (Interval in Earth days: 1298)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.68

273.

-8.3

-25.5

42.4

39.6


  


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