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.

Channels in Northeastern Hellas Planitia:   ESP_073701_1480   ESP_082233_1480   (Interval in Earth days: 664)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.4

82.6

2.65

24.19

56.5

58.8

Rayed Impact Crater in Meridiani Planum:   ESP_073572_1785   ESP_073638_1785   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.56

0.52

-0.7

-20.9

57.4

59.0

Gullies on Pole-Facing Slope of Ice-Filled Crater:   ESP_073591_1385   ESP_073446_1385   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.9

206.

8.21

-8.15

59.6

62.9

Landslides inside Impact Crater:   ESP_073749_1860   ESP_073815_1860   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.745

207.

7.31

-11.9

58.3

59.8

Layered Rock in Hollow on Mesa-Top:   ESP_073607_1825   ESP_073673_1825   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.246

123.

8.32

-12.3

57.3

58.9

Highland Channels:   ESP_073604_1340   ESP_064780_1340   (Interval in Earth days: 687)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-45.8

215.

-23.

7.346

63.4

61.2

Ares Vallis Landform:   ESP_073639_1950   ESP_073916_1950   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.59

329.

-4.6

-18.6

61.8

63.7

Small Delta or Fan:   ESP_073679_1920   ESP_073824_1920   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.86

317.

3.07

23.89

60.4

59.1

Deposits in Ganges Chasma:   ESP_073732_1715   ESP_066491_1715   (Interval in Earth days: 564)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.58

311.

19.7

-7.10

54.3

43.8

Intersection of Aeolis Serpens with Crater Rim:   ESP_073870_1820   ESP_073527_1820   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.154

147.

-26.

8.608

60.0

57.3


  


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