Stereo Pairs 
An explanation of stereo pairs and their use (PDF)  

In addition to planned stereo pairs, the Pairendipity software can identify all overlapping images suitable for stereo processing. Global lists of such image pairs for the HiRISE and CTX datasets are provided here ordered by latitude. Images taken close together in time minimize illumination and frost differences and are especially useful (see the Delta-Days column). Stereo images planned within the same 14-day operations cycle are known as SPORCs.

Hydrated Sulfates in Melas Chasma:   ESP_082700_1670   ESP_082990_1670   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.7

290.

3.19

17.88

54.8

51.2

Topographic Interactions in Athabasca Valles:   ESP_082217_1895   ESP_082283_1895   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.431

156.

-1.6

-17.5

59.9

61.4

Terrain Sample:   ESP_082131_1830   ESP_082408_1830   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.782

343.

9.02

-2.09

57.9

59.0

Hematite-Rich Terrain in West Candor Chasma:   ESP_082120_1745   ESP_082331_1745   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.24

285.

-1.4

12.00

58.3

56.8

Ridges in Meridiani Planum:   ESP_082289_1805   ESP_082355_1805   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.516

351.

8.46

-7.68

57.8

59.0

Spiders with Large Spring Fans:   ESP_082112_0970   ESP_082113_0970   (Interval in Earth days: 0)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-82.8

167.

4.86

-29.9

83.5

86.8

Distributary Channels of Athabasca Valles:   ESP_082415_1880   ESP_082349_1880   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.786

154.

-29.

-7.03

62.5

60.4

Mound in Chryse Planitia:   ESP_082303_2085   ESP_082158_2085   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.34

323.

28.5

6.38

63.5

64.0

Hillslope Morphologies in Rim of Vinogradov Crater:   ESP_082211_1615   ESP_082277_1615   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.1

323.

5.12

-11.5

58.1

58.9

Partly-Filled Impact Crater near Nicholson Crater:   ESP_082176_1830   ESP_082242_1830   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.848

196.

-7.6

-23.2

59.3

60.7


  


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