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.

Blocky Deposit and Valley Networks Along Melas Chasma Wallrock:   PSP_007443_1705   PSP_007733_1705   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.17

282.

-9.1

5.346

49.8

52.0

Landforms in Eastern Amazonis Planitia:   PSP_008131_1930   PSP_008421_1930   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
12.68

213.

-6.4

3.766

45.6

46.2

Bright Layers in Columbus Crater:   PSP_007710_1500   PSP_008066_1500   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.6

193.

6.36

-4.46

64.8

69.2

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

Unnamed Well-Preserved Crater in Terra Cimmeria:   PSP_007000_1475   PSP_007145_1475   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.0

141.

-1.0

10.11

57.0

58.6

Gullies and Bedrock Exposures in Impact Crater Wall:   PSP_008153_1480   PSP_009155_1480   (Interval in Earth days: 78)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.4

337.

4.51

-12.3

70.8

76.3

Flow Feature on Eos Chasma Wall:   PSP_007389_1665   ESP_026324_1665   (Interval in Earth days: 1475)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.4

317.

-2.5

19.41

51.1

59.2

Interesting Periglacial Assemblage in Utopia Planitia:   PSP_007384_2225   PSP_009467_2225   (Interval in Earth days: 163)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.22

86.3

-1.0

14.43

44.2

43.1

Cratered Cones in Isidis Planitia:   PSP_007872_1900   PSP_009586_1900   (Interval in Earth days: 134)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.820

85.7

-6.6

-23.4

45.1

52.9

Santa Fe Crater in Chryse Planitia:   PSP_007244_1995   ESP_016052_1995   (Interval in Earth days: 687)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.19

311.

5.51

19.74

38.9

37.5


  


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