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.

South Polar Troughs:   ESP_083993_0940   ESP_084045_0940   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-86.1

308.

5.53

20.25

64.6

63.6

Depression near Terminus of Lobate Deposit in Argyre Region:   ESP_083780_1330   ESP_083846_1330   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.7

327.

4.09

-15.7

42.6

43.6

Lethe Vallis Features:   ESP_083852_1845   ESP_084076_1845   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.307

155.

-8.8

26.04

51.6

46.6

Sulfate-Rich South Polar Region Cryptic Terrain in Aram Chaos:   ESP_083898_1830   ESP_084267_1830   (Interval in Earth days: 29)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.117

340.

-15.

20.01

50.9

44.0

Hale Crater Central Peak Slopes:   ESP_084057_1445   ESP_057906_1445   (Interval in Earth days: 2038)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.3

323.

-16.

0

39.5

32.9

Crater with Hydration Signatures in West Hellas Planitia:   ESP_083988_1400   ESP_084568_1400   (Interval in Earth days: 45)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.7

47.2

-0.7

13.85

39.6

37.9

Light Layers at Base of Mounds in Oxia Colles:   ESP_084096_2010   ESP_084320_2010   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.63

330.

-8.3

22.19

59.3

54.8

Complex Dune in Thaumasia Region:   ESP_083847_1360   ESP_083913_1360   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.7

297.

0.89

-19.1

41.4

42.5

Scarp Monitoring:   ESP_083854_1295   ESP_075243_1295   (Interval in Earth days: 671)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-50.1

106.

9.52

-2.48

42.9

42.7

Sinuous Ridges and Lobate Debris Aprons on Edge of Argyre Planitia:   ESP_083886_1235   ESP_084097_1235   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-56.0

314.

5.91

-9.43

45.4

46.0


  


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