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.

Fresh 10-Kilometer Diameter Unnamed Crater in Terra Sabaea:   PSP_007966_1615   ESP_025055_1615   (Interval in Earth days: 1331)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.1

41.5

5.02

25.73

59.9

51.0

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

Wall Layers of Tooting Crater:   PSP_007907_2035   ESP_019115_2035   (Interval in Earth days: 873)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.18

208.

-2.3

5.434

41.6

48.0

Slope Streaks Beginning at Stratigraphic Layers:   PSP_007473_1850   PSP_008264_1850   (Interval in Earth days: 62)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.996

181.

-5.4

5.46

43.6

48.7

Light-Toned Rock Exposures:   PSP_007101_1730   ESP_019311_1730   (Interval in Earth days: 952)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.99

260.

-7.9

3.361

44.7

56.7

Small Shield Volcano in Ceraunius Fossae Region:   PSP_008156_2005   ESP_016094_2005   (Interval in Earth days: 618)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.13

249.

-1.8

-23.6

43.0

41.3

Potential Chloride Salts:   PSP_007032_1665   ESP_011317_1665   (Interval in Earth days: 334)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.1

345.

-3.1

26.53

46.4

56.6

Well-Peserved Large Crater with Central Peak and Pit:   PSP_007366_1360   ESP_024732_1360   (Interval in Earth days: 1353)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.4

229.

2.46

-27.4

70.5

67.3

Unnamed Small Rayed Crater in Hesperia Region:   PSP_008135_1520   PSP_008425_1520   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.9

108.

-4.0

6.037

68.6

70.2

Clinoforms in Melas Chasma:   PSP_007878_1700   PSP_008735_1700   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.75

283.

4.89

-23.0

53.8

61.4


  


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