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.

Upper Section of Northern Olympus Mons Basal Scarp:   PSP_007445_2035   PSP_008447_2035   (Interval in Earth days: 78)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.90

223.

-1.4

-13.8

40.1

44.4

Naar Crater:   PSP_007046_2030   ESP_025691_2030   (Interval in Earth days: 1453)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.90

317.

3.89

-21.5

39.0

42.0

Floor and Central Uplift of Mazamba Crater in Thaumasia Planum:   PSP_007100_1520   ESP_033248_1520   (Interval in Earth days: 2038)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.5

290.

-1.6

-23.6

55.6

51.8

Region Showing Differentially-Eroded Distal Fan Deposits:   PSP_007688_1575   PSP_008545_1575   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.0

72.9

6.99

-15.6

59.4

68.1

Perplexing Landforms on Hellas Basin Floor:   PSP_007135_1400   ESP_016088_1400   (Interval in Earth days: 698)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.4

56.8

-4.2

16.93

64.5

65.2

Western Half of Central Peak of Large Well-Preserved Crater:   PSP_007857_1475   PSP_010006_1475   (Interval in Earth days: 168)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.0

140.

-6.7

19.27

68.9

72.7

Crater with Multiple Gully Orientations:   PSP_007001_2200   PSP_007937_2200   (Interval in Earth days: 73)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.48

105.

-8.6

6.751

45.7

41.3

Knobs and Cones in Acidalia Planitia:   PSP_007506_2220   ESP_051759_2220   (Interval in Earth days: 3448)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.57

354.

3.16

20.33

43.2

38.9

Flow-Banded Deformed Terrain of Hellas Basin Floor:   PSP_007201_1405   PSP_007491_1405   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.9

54.9

-7.0

3.906

65.3

68.9

Central Peak of Large 40-Kilometer Diameter Crater:   PSP_007592_1995   ESP_045595_1995   (Interval in Earth days: 2961)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.25

169.

-0.9

19.06

40.8

43.5


  


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