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.

Pit in Residual Ice Cap:   ESP_083943_0920   ESP_074975_0920   (Interval in Earth days: 699)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.0

232.

19.1

29.01

64.7

63.6

Narrow South Polar Carbon Dioxide Deposit:   ESP_083891_0920   ESP_075490_0920   (Interval in Earth days: 655)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.0

211.

19.1

29.16

64.6

66.4

Depression near Terminus of Lobate Deposit in Argyre Region:   ESP_083780_1330   ESP_083846_1330   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.7

327.

4.09

-15.7

42.6

43.6

Inverted Channel in Arabia Terra:   ESP_083792_1895   ESP_083726_1895   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.630

354.

-24.

1.823

56.6

55.5

Sinuous Ridges and Lobate Debris Aprons on Edge of Argyre Planitia:   ESP_083886_1235   ESP_084097_1235   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-56.0

314.

5.91

-9.43

45.4

46.0

Measure Heights and Widths of Raised Ridges in Sedimentary Deposit:   ESP_083866_1560   ESP_084367_1560   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.5

135.

4.74

-11.7

39.7

36.5

Irregular Rings and Hills:   ESP_084075_2080   ESP_084444_2080   (Interval in Earth days: 29)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.88

182.

-5.1

28.45

64.7

58.1

Crater Rim Breach:   ESP_083932_1715   ESP_084657_1715   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.28

131.

0.56

21.48

43.7

34.7

Light Layers at Base of Mounds in Oxia Colles:   ESP_084096_2010   ESP_084320_2010   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.63

330.

-8.3

22.19

59.3

54.8

Troughs Overlying South Polar Layered Deposit:   ESP_083964_0915   ESP_083635_0915   (Interval in Earth days: 25)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.4

10.6

23.8

19.82

64.7

64.8


  


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