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.

Central Pit of Large Crater South of Valles Marineris:   PSP_007047_1640   PSP_010264_1640   (Interval in Earth days: 251)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.9

296.

-7.3

5.642

48.3

63.0

Interior Channel in Durius Valles:   PSP_007012_1630   PSP_007157_1630   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-16.8

171.

-3.9

8.48

48.0

49.2

Distal Rampart of Crater in Isidis Region:   PSP_007740_1920   ESP_016047_1920   (Interval in Earth days: 647)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
12.01

89.5

-2.3

18.67

43.2

38.0

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

Cones and Pitted Material Inside An Embayed Crater in the Tartarus Montes:   PSP_007605_2055   PSP_007961_2055   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.39

173.

4.99

-5.25

40.0

41.8

Etched Terrain with Possible Layering West of Juventae Chasma:   PSP_007482_1760   PSP_009486_1760   (Interval in Earth days: 156)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.20

296.

1.06

-9.01

47.0

58.5

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

Deposits in Kasei Valles:   PSP_007970_2015   ESP_033551_2015   (Interval in Earth days: 1993)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.06

287.

-0.6

17.86

42.0

36.8

Layering in Uzer Crater Wall Seen in MOC Image E01-00244:   PSP_008073_1785   PSP_009721_1785   (Interval in Earth days: 128)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.27

358.

-2.0

13.86

51.2

55.4

Gullies on South-Facing Wall of Crater:   PSP_007045_1450   ESP_016130_1450   (Interval in Earth days: 708)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.6

353.

-5.7

-23.5

59.8

64.8


  


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