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.

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

Knobs and Valley Fill in Nilosyrtis Region:   PSP_009824_2190   PSP_010536_2190   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.51

61.6

3.59

17.45

46.0

51.4

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

Medusae Fossae Formation and Cratered Cemented Dunes:   PSP_009609_1675   PSP_010453_1675   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.5

178.

5.31

-18.9

62.4

62.6

Fresh 8-Kilometer Diameter Impact Crater:   PSP_009625_1900   ESP_016060_1900   (Interval in Earth days: 501)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.793

98.5

4.97

-22.4

50.7

41.9

Light-Toned Deposits and Possible Fluvial Channels on Floor of Ius Chasma:   PSP_010146_1720   PSP_010568_1720   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.96

277.

-4.7

-18.8

59.9

60.5

High-Latitude Exposure of North Polar Layered Deposits:   PSP_009309_2725   PSP_009589_2675   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.52

327.

-4.7

-14.4

64.2

64.4

Exposure of Polar Layered Deposits in Area Not Well Observed:   PSP_009359_2715   PSP_009400_2685   (Interval in Earth days: 3)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
88.42

42.9

-12.

-12.2

64.8

64.2

Exposure of Polar Layered Deposits:   PSP_010116_2680   PSP_010075_2720   (Interval in Earth days: 3)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
88.20

303.

-10.

-10.3

69.5

69.6

Central Peak of Crater:   PSP_009561_2325   PSP_010260_2325   (Interval in Earth days: 54)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
52.40

39.8

0.54

-21.0

46.6

54.9


  


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