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.

Seasonal Monitoring:   PSP_005455_0975   PSP_005547_0975   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-82.1

225.

1.30

15.98

69.4

69.9

Apparent Fluvial Channel at the Summit of Hecates Tholus:   PSP_004982_2120   PSP_005259_2120   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
31.70

150.

-3.6

-27.4

63.0

60.7

Layered Rock Outcrops in West Candor Chasma:   PSP_005742_1750   PSP_006665_1750   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.93

285.

1.77

-8.25

33.5

39.1

Channels or Flow Features with Inverted Topography on Arsia Mons:   PSP_005915_1720   ESP_011690_1720   (Interval in Earth days: 450)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.81

242.

-5.1

8.736

33.9

56.6

Possible Collapse Feature in Impact Crater Ejecta:   PSP_005933_2200   ESP_011286_2200   (Interval in Earth days: 417)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.71

105.

-6.4

11.69

56.3

62.4

Gullies in Palikir Crater:   PSP_005943_1380   ESP_011428_1380   (Interval in Earth days: 427)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.5

202.

3.28

-12.4

45.9

67.3

Fresh Crater on Edge of South Polar Layered Deposits:   PSP_005457_0995   PSP_005760_0995   (Interval in Earth days: 24)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-80.5

167.

0.47

16.95

68.1

71.9

Possible Pingo at the Border Between Fretted Crater Ejecta:   PSP_006632_2240   PSP_010337_2240   (Interval in Earth days: 288)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.79

98.7

1.07

-21.5

50.4

53.6

South Polar Layered Deposits Survey:   PSP_005302_0880   PSP_005801_0920   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.7

153.

6.38

18.16

73.1

78.7

Basal Scarp of South Polar Layered Deposits:   PSP_004759_0955   ESP_013897_0955   (Interval in Earth days: 712)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-84.4

156.

0

-14.1

64.0

68.0


  


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