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.

Floor of Cut Crater:   ESP_016461_1680   ESP_025533_1680   (Interval in Earth days: 707)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.8

312.

-6.7

15.71

53.1

53.0

Layers Exposed in Wall of Crater in the Floor of Hydaspis Chaos:   ESP_016513_1850   ESP_017502_1850   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.146

329.

3.09

-12.0

44.4

51.1

Volcanic Features in Ceraunius Fossae Region:   ESP_016661_2020   ESP_017096_2020   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.86

248.

-16.

25.35

42.3

40.1

Gale Crater Layers in Northeast Section of Mound with Possible Sulfates:   ESP_016586_1755   ESP_016731_1755   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.64

138.

0.77

18.24

49.8

49.8

Possible MSL Landing Site in Syrtis Major:   ESP_016364_1980   ESP_016219_1980   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.89

77.2

-14.

-27.6

41.5

42.2

Chaos on the Floor of Candor Chasma:   ESP_016686_1735   ESP_017108_1735   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.49

287.

10.2

-4.71

51.1

55.2

Terrain South of Newcomb Crater:   ESP_016736_1520   ESP_068970_1525   (Interval in Earth days: 4070)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.6

5.59

4.65

-7.50

65.7

63.9

Fresh Multiple Impact:   ESP_016718_2005   ESP_018353_2005   (Interval in Earth days: 127)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.26

131.

0.06

15.40

41.3

44.6

Zunil Crater Secondary Crater Cluster:   ESP_016796_1830   ESP_016941_1830   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.871

164.

-8.6

7.724

48.3

48.1

Fresh Crater on Alba Patera:   ESP_016371_2235   ESP_016226_2235   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.05

240.

4.58

-7.09

43.2

44.8


  


Page 683 of 873 (8,724 images)