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.

Recent Crater in Southern Mid-Latitudes:   ESP_066067_1350   ESP_066476_1350   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-44.6

8.27

-1.5

-22.4

44.2

43.5

South Polar Layered Deposits:   ESP_066063_0940   ESP_066062_0940   (Interval in Earth days: 0)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-86.0

161.

0.05

20.37

64.9

63.1

South Polar Cap Vertical Change Monitoring:   ESP_065909_0930   ESP_065989_0930   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-86.7

16.2

23.3

8.954

63.8

64.7

Layering in Arabia Terra:   ESP_065922_1850   ESP_065988_1850   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.104

357.

7.70

-6.41

55.1

55.5

Ridges along Pavonis Mons Caldera Rim:   ESP_065992_1810   ESP_073853_1810   (Interval in Earth days: 612)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.999

248.

6.46

17.64

52.4

56.1

Possible Sulfate-Rich Terrain:   ESP_065964_1720   ESP_065898_1720   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.74

294.

-8.1

6.721

49.7

49.3

Scarps in Icaria Region:   ESP_065716_1420   ESP_065373_1420   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.9

227.

-11.

6.851

47.9

51.1

Gully Monitoring and Topography:   ESP_066072_1375   ESP_065175_1375   (Interval in Earth days: 70)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.9

232.

-10.

6.942

44.4

54.5

Layered Rocks of Ophir Mensa:   ESP_065740_1760   ESP_065806_1760   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.19

285.

8.68

-7.23

52.1

52.6

Hydrated Sulfate-Rich Terrain in Aram Chaos:   ESP_066081_1830   ESP_092930_1830   (Interval in Earth days: 2092)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.992

339.

-0.1

-20.4

53.1

48.0


  


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