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.

Potential Phyllosilicates in Acidalia Region:   PSP_009182_2215   PSP_009472_2215   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.28

309.

-4.4

16.00

43.6

43.0

Exposure of Polar Layered Deposits Not Well Observed by Previous Missions:   PSP_009039_2680   PSP_009133_2680   (Interval in Earth days: 8)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
88.00

169.

-8.0

-15.3

63.1

63.0

Impact Crater Amid the Deuteronilus Mensae:   PSP_009021_2245   PSP_009654_2245   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.21

23.3

8.73

-7.10

42.2

46.4

Landslides in Ganges Chasma:   PSP_009037_1715   PSP_009538_1715   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.54

315.

-14.

7.943

60.9

59.8

Zunil Crater Ray Formed within a Dusty Region:   PSP_008225_1830   ESP_018510_1830   (Interval in Earth days: 801)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.916

167.

-2.7

16.38

50.1

51.7

Layered Deposits in Crater in Arabia Terra:   PSP_008520_2085   PSP_009232_2085   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.00

27.9

1.13

-16.8

42.3

45.8

Merging Lobate Debris Aprons of Deuteronilus Mensae:   PSP_008744_2240   PSP_009535_2240   (Interval in Earth days: 62)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.76

29.3

-6.2

15.83

43.0

43.5

Stratigraphy Exposed in Crater Wall:   PSP_009048_1965   PSP_010037_1965   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.47

11.6

-4.7

-17.5

47.5

51.5

Central Peak of Bonestell Crater:   PSP_008733_2225   ESP_018372_2225   (Interval in Earth days: 752)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.96

329.

-2.7

11.77

42.5

43.0

Unnamed Faded Rayed Crater in Elysium Planitia:   PSP_009123_2040   ESP_016560_2040   (Interval in Earth days: 579)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.94

122.

3.65

21.08

44.6

38.5


  


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