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 5-Kilometer Diameter Crater:   PSP_009532_1640   PSP_010033_1640   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.6

121.

-7.7

17.88

65.2

62.7

Exposure of North Polar Layered Deposits for Stratigraphic Analysis:   PSP_009999_2670   PSP_010132_2670   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
86.94

279.

-5.6

-20.5

67.0

69.1

Exposure of Polar Layered Deposits in Area Not Well Observed:   PSP_009347_2715   PSP_009388_2685   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
88.72

12.7

-15.

-15.5

64.8

64.4

Debris Flow in Juventae Chasma:   PSP_010198_1755   ESP_016290_1755   (Interval in Earth days: 474)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.25

297.

0.26

22.12

57.8

45.2

Potential Paleolake in Crater in Ophir Planum:   PSP_010290_1700   PSP_010435_1700   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.0

306.

0.86

17.82

60.3

58.8

Flow on Floor of Kasei Valles:   PSP_010000_2055   ESP_069104_2055   (Interval in Earth days: 4605)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.17

299.

0

22.72

48.1

44.8

Seasonal Monitoring of Polar Crater with Summer Ice:   PSP_009364_2505   ESP_018766_2505   (Interval in Earth days: 732)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
70.05

13.8

-2.3

-22.2

52.5

58.1

Possible Flute Casts in Ares Vallis:   PSP_009722_1960   PSP_009867_1960   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.92

329.

2.51

17.22

48.9

48.1

Small Shield Covering the Noctis Fossae:   PSP_010305_1780   PSP_010661_1780   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.91

256.

-7.0

-0.74

57.3

56.9

Possible Collapsed Pingos in Utopia Planitia:   PSP_009704_2190   PSP_010192_2190   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.40

97.8

3.34

-21.0

45.3

51.2


  


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