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.

Terrain Northwest of Hellas Planitia:   ESP_019543_1465   ESP_019899_1465   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.1

50.7

0

11.96

68.5

64.4

Channels and Vents in Tharsis Region:   ESP_019483_2010   ESP_019549_2010   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.54

241.

2.59

-17.9

50.9

53.1

Fresh 3-Kilometer Diameter Crater in Terra Sabaea:   ESP_019544_1675   ESP_020177_1675   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.3

20.1

7.71

-6.37

58.0

56.7

Light-Toned Outcrops in Noctis Region:   ESP_019324_1725   ESP_019469_1725   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.62

266.

-5.6

11.59

57.6

56.1

Ismenius Cavus:   ESP_019333_2140   ESP_019478_2140   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.77

16.9

-14.

-2.15

51.9

52.3

Western Half of Crater in Sinus Sabaeus:   ESP_019307_1715   ESP_019808_1715   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.50

12.3

-21.

6.908

59.3

56.0

Fissures in Tempe Terra:   ESP_019508_2245   ESP_019574_2245   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.91

276.

-3.8

-18.2

55.2

57.3

Wavy Stratification Features in Crater Wall in MOC Image S14-00005:   ESP_019558_1800   ESP_020125_1800   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.165

357.

-10.

0.304

55.2

54.8

Cones in Isidis Planitia:   ESP_019291_1965   ESP_019924_1965   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.59

82.7

17.0

3.208

48.8

54.0

Pit on the Eastern Flank of Pavonis Mons:   ESP_019351_1795   ESP_019984_1795   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.45

248.

-2.8

-17.6

54.7

56.1


  


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