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.

Fretted Terrain :   ESP_028613_1375   ESP_028758_1375   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-42.0

116.

-5.6

5.302

70.5

68.1

Light-Toned Deposits in Ladon Valles Basin :   ESP_028816_1605   ESP_029594_1605   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.2

329.

6.81

-3.96

57.8

53.2

IR-Distinct Crater :   ESP_028676_2185   ESP_054152_2185   (Interval in Earth days: 1986)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.06

185.

-2.3

-20.3

57.5

46.8

Crater Filled with Mantling Deposit in Far Eastern Acidalia Planitia :   ESP_028628_2315   ESP_028694_2315   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
51.20

54.1

-4.9

-17.8

61.8

64.0

Exhumed Fan in Nilosyrtis Mensae :   ESP_028680_2070   ESP_028825_2070   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
26.90

76.8

7.55

18.85

53.9

54.5

Crater Ejecta Margin :   ESP_028600_2255   ESP_046204_2255   (Interval in Earth days: 1371)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
45.03

99.4

-3.0

7.704

58.8

55.5

Deformed Crater on Huygens Crater Floor :   ESP_028826_1645   ESP_028760_1645   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.4

56.3

5.64

27.53

56.7

55.2

Arsia Mons Southern Caldera Wall Upper Flank and Caldera Floor :   ESP_028872_1695   ESP_082280_1695   (Interval in Earth days: 4161)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.1

239.

6.91

-4.71

55.2

58.1

Crater Rim Near Eumenides Dorsum :   ESP_028623_1870   ESP_055510_1870   (Interval in Earth days: 2095)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.917

196.

-5.7

-28.8

53.5

55.4

Ravines in Melas Chasma :   ESP_028633_1695   ESP_034382_1695   (Interval in Earth days: 448)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.1

285.

4.17

18.51

56.0

53.0


  


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