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 of Polar Crater with Summer Ice:   PSP_009364_2505   ESP_018766_2505   (Interval in Earth days: 732)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
70.05

13.8

-2.3

-22.2

52.5

58.1

High-Latitude Exposure of North Polar Layered Deposits:   PSP_009584_2675   PSP_009757_2675   (Interval in Earth days: 13)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.31

77.4

-4.6

-21.6

64.0

65.8

Possible Pingos in Gusev Crater:   PSP_009385_1655   PSP_009886_1655   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.2

175.

-18.

5.226

65.1

63.0

Unconformity in Gemini Lingula Layered Deposits:   PSP_009482_2605   PSP_009878_2605   (Interval in Earth days: 31)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.31

22.5

-0.8

-19.1

58.4

62.7

Slope Streaks on Nicholson Crater Mound:   PSP_009371_1800   PSP_009516_1800   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.00

195.

-5.9

9.471

55.9

55.0

North Polar Layered Deposits Bench:   PSP_009991_2655   PSP_010109_2655   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
85.23

165.

-13.

0.284

66.2

66.7

Aprons with Channels in Eos Chasma:   PSP_009327_1665   PSP_009960_1665   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.3

317.

0

-20.9

63.3

64.2

Cluster of Craters and Edifices on Top of Mesa:   PSP_009642_2215   PSP_010143_2215   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.10

350.

-1.2

16.64

45.5

47.8

A North Polar Crater:   PSP_009689_2645   PSP_010084_2645   (Interval in Earth days: 31)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.33

120.

-1.7

12.07

62.3

65.3

North Polar Terrain:   PSP_009914_2750   PSP_010682_2650   (Interval in Earth days: 59)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.90

334.

0

18.02

69.7

73.7


  


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