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.

Interaction of Modified Ejecta with Tectonic Features in Ascuris Planum :   ESP_045525_2235   ESP_045248_2235   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.98

278.

6.02

19.25

45.9

42.3

Crater with Persistent Ice :   ESP_045503_2540   ESP_045160_2540   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
73.88

152.

-3.1

6.7

60.7

56.4

Exposure of North Polar Layered Deposits :   ESP_045625_2615   ESP_045599_2615   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
81.24

44.7

8.37

-6.57

66.3

66.7

Dunes Buried by Water Ice :   ESP_045592_2625   ESP_045777_2625   (Interval in Earth days: 14)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
82.30

223.

6.95

-7.67

66.6

69.9

Fractured Crater Fill :   ESP_045522_2175   ESP_045588_2175   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.97

1.48

8.69

-9.68

44.3

46.6

Breached Crater Near Marte Vallis :   ESP_045634_2035   ESP_045924_2035   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.36

185.

6.26

26.04

44.5

45.0

65-Meter Diameter Crater on North Residual Ice :   ESP_045448_2730   ESP_062893_2730   (Interval in Earth days: 1360)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
86.98

98.2

-1.4

-10.6

71.2

70.1

Lava Channel in Eastern Amazonis Planitia :   ESP_045765_1995   ESP_046187_1995   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.13

210.

-0.0

-18.6

46.2

51.0

Floor of Maja Valles :   ESP_045564_1860   ESP_046131_1860   (Interval in Earth days: 45)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.044

299.

4.54

-6.00

47.7

50.0

Volcanic Flow Features in Southern Elysium Planitia :   ESP_045793_1775   ESP_050975_1775   (Interval in Earth days: 404)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.25

167.

6.27

-8.27

50.7

37.7


  


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